This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:36:11.19 +38:20:58.6
86.08887 -10.17787 galactic Cyg Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:11.19 +38:20:58.6 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.060 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:11.19 +38:20:58.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:11.19 +38:20:58.6: 14.33 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:42:02.26 +37:42:53.1
86.51948 -11.42351 galactic Cyg Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5073+37.7138 | 21:42:02.26 +37:42:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.052 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:02.26 +37:42:53.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:02.26 +37:42:53.1: 14.56 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5073+37.7138,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5073+37.7138 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:40:31.53 +37:49:27.5
86.36792 -11.14206 galactic Cyg Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:31.53 +37:49:27.5 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:31.53 +37:49:27.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:31.53 +37:49:27.5: 14.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:42:44.12 +39:07:51.7
87.58373 -10.45774 galactic Cyg Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:44.12 +39:07:51.7 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:44.12 +39:07:51.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:44.12 +39:07:51.7: 15.11 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.53 21:31:17.47 +37:57:30.7
85.10568 -9.80171 galactic Cyg Second-epoch detections are separated by 2.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8242+37.9583 | 21:31:17.47 +37:57:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:17.47 +37:57:30.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:17.47 +37:57:30.7: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.8242+37.9583,2461185.8480,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.8242+37.9583 20260525.3480 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:41:56.61 +38:52:29.8
87.29369 -10.54672 galactic Cyg Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:56.61 +38:52:29.8 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.325+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:56.61 +38:52:29.8: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:56.61 +38:52:29.8: 14.62 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:40:17.04 +41:25:00.8
88.77088 -8.43970 galactic Cyg Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:17.04 +41:25:00.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.508+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:17.04 +41:25:00.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:17.04 +41:25:00.8: 14.41 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.33 21:29:26.32 +37:55:00.9
84.80971 -9.57804 galactic Cyg Second-epoch detections are separated by 3.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.3596+37.9165 | 21:29:26.32 +37:55:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.697+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:26.32 +37:55:00.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:26.32 +37:55:00.9: 14.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.3596+37.9165,2461185.8480,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.3596+37.9165 20260525.3480 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.66 21:56:23.29 +38:47:33.2
89.42427 -12.43347 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:23.29 +38:47:33.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:23.29 +38:47:33.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:23.29 +38:47:33.2: 14.56 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.53 21:42:39.45 +37:40:34.5
86.58647 -11.53399 galactic Cyg Second-epoch detections are separated by 3.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:39.45 +37:40:34.5 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.048 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:39.45 +37:40:34.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:39.45 +37:40:34.5: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 21:39:10.96 +36:29:08.3
85.24533 -11.95070 galactic Cyg Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:10.96 +36:29:08.3 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.055 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:10.96 +36:29:08.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:10.96 +36:29:08.3: 14.13 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:45:01.35 +40:16:55.6
88.69140 -9.88346 galactic Cyg Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2656+40.2795 | 21:45:01.35 +40:16:55.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.445+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:01.35 +40:16:55.6: 13.52 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:01.35 +40:16:55.6: 14.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2656+40.2795,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2656+40.2795 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:29:04.98 +34:49:01.3
82.55166 -11.74388 galactic Cyg Second-epoch detections are separated by 3.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:04.98 +34:49:01.3 (user input) | T | P | (position from user input) J-Ks=0.788+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:04.98 +34:49:01.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:04.98 +34:49:01.3: 14.34 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 22:06:13.56 +41:38:26.9
92.72725 -11.34220 galactic Lac Second-epoch detections are separated by 2.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.5562+41.6426 | 22:06:13.56 +41:38:26.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.435+/-0.051 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:13.56 +41:38:26.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:13.56 +41:38:26.9: 14.49 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.5562+41.6426,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.5562+41.6426 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:36:57.17 +34:14:37.0
83.33878 -13.28185 galactic Cyg Second-epoch detections are separated by 1.5" and 4.1 pix
The object was found in VSX25" Gaia DR3 1950258238673610496
Type: RS
# Max. Min./Amp. JD0 Period
14.620 G 14.710 G 1.899440000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:57.17 +34:14:37.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:57.17 +34:14:37.0: 14.76 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950258238673610496,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950258238673610496 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:34:02.89 +36:28:38.6
84.46962 -11.25221 galactic Cyg Second-epoch detections are separated by 1.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.5196+36.4730 | 21:34:02.89 +36:28:38.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.492+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:02.89 +36:28:38.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:02.89 +36:28:38.6: 13.90 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.5196+36.4730,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.5196+36.4730 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:50:37.07 +36:00:47.8
86.69282 -13.83409 galactic Peg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.6650+36.0068 | 21:50:37.07 +36:00:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.415+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:37.07 +36:00:47.8: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:37.07 +36:00:47.8: 15.02 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.6650+36.0068,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.6650+36.0068 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.33 21:34:54.31 +35:45:43.1
84.09530 -11.89041 galactic Cyg Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.7303+35.7597 | 21:34:54.31 +35:45:43.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:54.31 +35:45:43.1: 13.27 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:54.31 +35:45:43.1: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.7303+35.7597,2461185.8480,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.7303+35.7597 20260525.3480 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:33:31.70 +37:30:03.8
85.11020 -10.43805 galactic Cyg Second-epoch detections are separated by 5.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.3904+37.4982 | 21:33:31.70 +37:30:03.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:31.70 +37:30:03.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:31.70 +37:30:03.8: 14.36 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.3904+37.4982,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.3904+37.4982 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:35:45.33 +33:50:35.9
82.87076 -13.40177 galactic Cyg Second-epoch detections are separated by 1.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:45.33 +33:50:35.9 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:45.33 +33:50:35.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:45.33 +33:50:35.9: 14.20 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.35 21:49:28.07 +34:19:21.2
85.36814 -14.95995 galactic Peg Second-epoch detections are separated by 2.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:28.07 +34:19:21.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:28.07 +34:19:21.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:28.07 +34:19:21.2: 14.38 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:51:47.59 +36:45:22.7
87.37375 -13.42164 galactic Cyg Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:47.59 +36:45:22.7 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:47.59 +36:45:22.7: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:47.59 +36:45:22.7: 14.71 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:43:20.61 +36:54:41.3
86.16974 -12.19518 galactic Cyg Second-epoch detections are separated by 1.7" and 3.5 pix
The object was found in VSX25" Gaia DR3 1952631637600503680
Type: ROT
# Max. Min./Amp. JD0 Period
13.120 G 13.150 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:20.61 +36:54:41.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:20.61 +36:54:41.3: 14.25 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952631637600503680,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952631637600503680 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:28:45.26 +36:42:07.2
83.84963 -10.35290 galactic Cyg Second-epoch detections are separated by 3.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:45.26 +36:42:07.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:45.26 +36:42:07.2: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:45.26 +36:42:07.2: 14.66 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.20 21:36:54.42 +37:55:38.1
85.90250 -10.58389 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:54.42 +37:55:38.1 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:54.42 +37:55:38.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:54.42 +37:55:38.1: 14.04 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:47:02.34 +36:41:21.7
86.58712 -12.85137 galactic Cyg Second-epoch detections are separated by 2.7" and 3.9 pix
The object was found in VSX22" Gaia DR3 1952470005090148864
Type: ROT
# Max. Min./Amp. JD0 Period
12.990 G 13.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:02.34 +36:41:21.7: 12.75 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:02.34 +36:41:21.7: 14.53 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952470005090148864,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952470005090148864 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:36:56.43 +36:30:10.2
84.91943 -11.63198 galactic Cyg Second-epoch detections are separated by 3.9" and 3.9 pix
The object was found in VSX 3" Gaia DR3 1951138324711432192
Type: ROT
# Max. Min./Amp. JD0 Period
14.560 G 14.590 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:56.43 +36:30:10.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:56.43 +36:30:10.2: 14.21 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951138324711432192,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951138324711432192 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:48:57.11 +38:28:35.3
88.07636 -11.74673 galactic Cyg Second-epoch detections are separated by 2.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:57.11 +38:28:35.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.766+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.11 +38:28:35.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.11 +38:28:35.3: 14.17 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:54:36.22 +36:42:13.8
87.78305 -13.82368 galactic Cyg Second-epoch detections are separated by 2.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:36.22 +36:42:13.8 (user input) | T | P | (position from user input) J-Ks=0.808+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:36.22 +36:42:13.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:36.22 +36:42:13.8: 14.24 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:54:21.74 +42:02:06.9
91.20144 -9.67267 galactic Cyg Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:21.74 +42:02:06.9 (user input) | T | P | (position from user input) J-Ks=0.454+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:21.74 +42:02:06.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:21.74 +42:02:06.9: 14.41 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 22:07:53.03 +37:40:43.6
90.54657 -14.70181 galactic Lac Second-epoch detections are separated by 2.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9789+37.6709 | 22:07:53.03 +37:40:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:53.03 +37:40:43.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:53.03 +37:40:43.6: 13.87 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9789+37.6709,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9789+37.6709 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 21:39:19.17 +36:37:29.1
85.36218 -11.86683 galactic Cyg Second-epoch detections are separated by 1.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:19.17 +36:37:29.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:19.17 +36:37:29.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:19.17 +36:37:29.1: 14.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:39:17.12 +36:38:31.8
85.36906 -11.84937 galactic Cyg Second-epoch detections are separated by 2.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:17.12 +36:38:31.8 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:17.12 +36:38:31.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:17.12 +36:38:31.8: 14.57 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 22:06:02.53 +38:59:35.1
91.06724 -13.43581 galactic Lac Second-epoch detections are separated by 1.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:02.53 +38:59:35.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:02.53 +38:59:35.1: 13.51 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:02.53 +38:59:35.1: 14.54 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:37:14.59 +37:16:14.3
85.49785 -11.11080 galactic Cyg Second-epoch detections are separated by 2.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:14.59 +37:16:14.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:14.59 +37:16:14.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:14.59 +37:16:14.3: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 22:00:25.81 +37:57:32.4
89.52285 -13.57939 galactic Lac Second-epoch detections are separated by 0.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:25.81 +37:57:32.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.456+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:25.81 +37:57:32.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:25.81 +37:57:32.4: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:58:37.95 +35:47:12.2
87.82971 -15.04795 galactic Peg Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:37.95 +35:47:12.2 (user input) | T | P | (position from user input) J-Ks=0.671+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:37.95 +35:47:12.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:37.95 +35:47:12.2: 14.76 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:45:21.68 +37:55:18.5
87.16091 -11.70426 galactic Cyg Second-epoch detections are separated by 1.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:21.68 +37:55:18.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.437+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:21.68 +37:55:18.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:21.68 +37:55:18.5: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:45:48.52 +34:00:26.9
84.56541 -14.69534 galactic Cyg Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:48.52 +34:00:26.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:48.52 +34:00:26.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:48.52 +34:00:26.9: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:46:11.76 +36:11:01.7
86.11424 -13.11972 galactic Cyg Second-epoch detections are separated by 1.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952347203385198464 | 21:46:12.42 +36:10:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.556+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:11.76 +36:11:01.7: 12.50 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:11.76 +36:11:01.7: 14.23 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952347203385198464,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952347203385198464 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:37:28.91 +34:32:02.1
83.62478 -13.14522 galactic Cyg Second-epoch detections are separated by 1.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:28.91 +34:32:02.1 (user input) | T | P | (position from user input) J-Ks=0.585+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:28.91 +34:32:02.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:28.91 +34:32:02.1: 14.60 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 21:27:14.01 +34:30:08.1
82.04952 -11.69928 galactic Cyg Second-epoch detections are separated by 2.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:14.01 +34:30:08.1 (user input) | T | P | (position from user input) J-Ks=13.323+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:14.01 +34:30:08.1: 12.92 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:14.01 +34:30:08.1: 14.18 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.13 21:37:12.18 +40:33:58.9
87.75794 -8.68067 galactic Cyg Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:12.18 +40:33:58.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:12.18 +40:33:58.9: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:12.18 +40:33:58.9: 13.81 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:42:26.08 +37:18:12.6
86.29898 -11.78222 galactic Cyg Second-epoch detections are separated by 2.6" and 3.5 pix
The object was found in VSX23" Gaia DR3 1952699944761506816
Type: VAR
# Max. Min./Amp. JD0 Period
16.860 G 17.090 G 0.014842900000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:26.08 +37:18:12.6: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:26.08 +37:18:12.6: 14.14 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952699944761506816,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952699944761506816 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:53:31.29 +36:34:23.1
87.52514 -13.78502 galactic Peg Second-epoch detections are separated by 0.5" and 3.7 pix
The object was found in VSX 1" ZTF J215331.21+363424.2
Type: EW
# Max. Min./Amp. JD0 Period
14.720 r Y 0.321 r 2458482.59580 0.363959000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:31.29 +36:34:23.1: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:31.29 +36:34:23.1: 14.35 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J215331.21+363424.2,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J215331.21+363424.2 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.13 21:28:13.25 +40:35:50.7
86.52510 -7.48922 galactic Cyg Second-epoch detections are separated by 1.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:13.25 +40:35:50.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:13.25 +40:35:50.7: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:13.25 +40:35:50.7: 14.02 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 21:54:04.90 +35:09:18.4
86.67382 -14.94407 galactic Peg Second-epoch detections are separated by 2.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:04.90 +35:09:18.4 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:04.90 +35:09:18.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:04.90 +35:09:18.4: 14.91 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 22:05:53.67 +41:23:38.0
92.52551 -11.50256 galactic Lac Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:53.67 +41:23:38.0 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:53.67 +41:23:38.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:53.67 +41:23:38.0: 14.60 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:57:44.02 +34:13:27.3
86.65363 -16.13976 galactic Peg Second-epoch detections are separated by 1.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:44.02 +34:13:27.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:44.02 +34:13:27.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:44.02 +34:13:27.3: 15.22 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.22 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 22:06:42.48 +40:57:13.5
92.38103 -11.94657 galactic Lac Second-epoch detections are separated by 0.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:42.48 +40:57:13.5 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:42.48 +40:57:13.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:42.48 +40:57:13.5: 15.03 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:45:30.42 +40:39:22.2
89.01084 -9.66139 galactic Cyg Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:30.42 +40:39:22.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:30.42 +40:39:22.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:30.42 +40:39:22.2: 14.53 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.22 21:36:23.81 +37:21:33.7
85.43379 -10.93126 galactic Cyg Second-epoch detections are separated by 4.0" and 4.3 pix
The object was found in VSX 3" Gaia DR3 1951998933077925248
Type: ROT
# Max. Min./Amp. JD0 Period
14.990 G 15.000 G 1.482740000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:23.81 +37:21:33.7: 13.52 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:23.81 +37:21:33.7: 14.87 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951998933077925248,2461185.8480,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951998933077925248 20260525.3480 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 22:01:48.10 +38:11:19.5
89.88724 -13.56624 galactic Lac Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:48.10 +38:11:19.5 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:48.10 +38:11:19.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:48.10 +38:11:19.5: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 22:08:28.75 +34:30:21.8
88.64839 -17.30028 galactic Peg Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:28.75 +34:30:21.8 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:28.75 +34:30:21.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:28.75 +34:30:21.8: 14.54 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 21:49:19.52 +40:40:24.4
89.58084 -10.11886 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:19.52 +40:40:24.4 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:19.52 +40:40:24.4: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:19.52 +40:40:24.4: 14.25 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:59:04.05 +35:55:55.0
87.99531 -14.99073 galactic Peg Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:04.05 +35:55:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:04.05 +35:55:55.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:04.05 +35:55:55.0: 14.35 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.22 21:32:18.87 +39:50:34.0
86.56825 -8.57470 galactic Cyg Second-epoch detections are separated by 2.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:18.87 +39:50:34.0 (user input) | T | P | (position from user input) J-Ks=0.721+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:18.87 +39:50:34.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:18.87 +39:50:34.0: 14.45 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 21:36:13.40 +36:37:41.9
84.89942 -11.44199 galactic Cyg Second-epoch detections are separated by 2.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:13.40 +36:37:41.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:13.40 +36:37:41.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:13.40 +36:37:41.9: 14.13 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 22:06:41.13 +40:11:40.3
91.91161 -12.55155 galactic Lac Second-epoch detections are separated by 1.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:41.13 +40:11:40.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:41.13 +40:11:40.3: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:41.13 +40:11:40.3: 14.45 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.25 22:10:06.42 +35:55:00.5
89.81597 -16.37726 galactic Lac Second-epoch detections are separated by 6.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:06.42 +35:55:00.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:06.42 +35:55:00.5: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:06.42 +35:55:00.5: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:57:21.05 +35:17:18.2
87.29374 -15.26863 galactic Peg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was found in VSX24" Gaia DR3 1948345840054926848
Type: ROT
# Max. Min./Amp. JD0 Period
18.200 G 18.350 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:21.05 +35:17:18.2: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:21.05 +35:17:18.2: 14.14 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948345840054926848,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948345840054926848 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.25 22:01:48.30 +39:56:07.0
90.99093 -12.19045 galactic Lac Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:48.30 +39:56:07.0 (user input) | T | P | (position from user input) J-Ks=0.807+/-0.105 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:48.30 +39:56:07.0: 12.83 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:48.30 +39:56:07.0: 14.31 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.11 21:58:11.17 +38:50:11.7
89.73180 -12.61916 galactic Lac Second-epoch detections are separated by 2.5" and 3.3 pix
The object was found in VSX19" Gaia DR3 1956069123264808320
Type: ROT
# Max. Min./Amp. JD0 Period
12.990 G 13.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:11.17 +38:50:11.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:11.17 +38:50:11.7: 13.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956069123264808320,2461185.8480,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956069123264808320 20260525.3480 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:35:46.01 +36:23:43.6
84.66861 -11.54912 galactic Cyg Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.9273+36.3931 | 21:35:46.01 +36:23:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.052 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:46.01 +36:23:43.6: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:46.01 +36:23:43.6: 14.59 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.9273+36.3931,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.9273+36.3931 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 22:09:10.00 +41:58:24.6
93.37843 -11.40071 galactic Lac Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:10.00 +41:58:24.6 (user input) | T | P | (position from user input) J-Ks=0.666+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:10.00 +41:58:24.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:10.00 +41:58:24.6: 14.49 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.16 21:35:14.10 +35:46:26.8
84.15349 -11.92758 galactic Cyg Second-epoch detections are separated by 1.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:14.10 +35:46:26.8 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:14.10 +35:46:26.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:14.10 +35:46:26.8: 14.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:53:18.52 +38:48:06.9
88.95569 -12.04565 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was found in VSX17" Gaia DR3 1953121229511946880
Type: ROT
# Max. Min./Amp. JD0 Period
15.200 G 15.240 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:18.52 +38:48:06.9: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:18.52 +38:48:06.9: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953121229511946880,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953121229511946880 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.10 21:48:40.82 +41:58:41.0
90.34035 -9.04377 galactic Cyg Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:40.82 +41:58:41.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.692+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:40.82 +41:58:41.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:40.82 +41:58:41.0: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.22 21:53:07.93 +40:37:52.5
90.11717 -10.61361 galactic Cyg Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.2751+40.6307 | 21:53:07.93 +40:37:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.449+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:07.93 +40:37:52.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:07.93 +40:37:52.5: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.2751+40.6307,2461185.8480,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.2751+40.6307 20260525.3480 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.17 22:02:56.32 +40:46:06.8
91.68659 -11.66345 galactic Lac Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:56.32 +40:46:06.8 (user input) | T | P | (position from user input) J-Ks=0.689+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:56.32 +40:46:06.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:56.32 +40:46:06.8: 14.10 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 22:00:26.34 +35:56:03.5
88.22068 -15.16316 galactic Peg Second-epoch detections are separated by 1.6" and 3.7 pix
The object was found in VSX 3" Gaia DR3 1948719918825623936
Type: ROT
# Max. Min./Amp. JD0 Period
14.850 G 14.870 G 7.700800000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:26.34 +35:56:03.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:26.34 +35:56:03.5: 13.70 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948719918825623936,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948719918825623936 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.02 21:51:26.79 +38:24:24.2
88.41108 -12.11583 galactic Cyg Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:26.79 +38:24:24.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:26.79 +38:24:24.2: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:26.79 +38:24:24.2: 13.90 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 21:41:11.94 +41:00:50.9
88.62965 -8.85481 galactic Cyg Second-epoch detections are separated by 3.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:11.94 +41:00:50.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:11.94 +41:00:50.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:11.94 +41:00:50.9: 13.87 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.06 21:50:25.25 +38:28:29.4
88.29904 -11.93426 galactic Cyg Second-epoch detections are separated by 2.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:25.25 +38:28:29.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.539+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:25.25 +38:28:29.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:25.25 +38:28:29.4: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 22:03:02.51 +36:29:37.6
89.00691 -15.05153 galactic Peg Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:02.51 +36:29:37.6 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:02.51 +36:29:37.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:02.51 +36:29:37.6: 14.10 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.04 21:46:04.46 +34:31:28.8
84.96327 -14.34583 galactic Cyg Second-epoch detections are separated by 3.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947677135125933568 | 21:46:07.29 +34:31:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:04.46 +34:31:28.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:04.46 +34:31:28.8: 14.09 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947677135125933568,2461185.8480,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947677135125933568 20260525.3480 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 22:00:22.58 +36:02:18.8
88.27802 -15.07391 galactic Peg Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:22.58 +36:02:18.8 (user input) | T | P | (position from user input) J-Ks=0.271+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:22.58 +36:02:18.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:22.58 +36:02:18.8: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.98 21:56:03.61 +38:29:55.7
89.18348 -12.62093 galactic Cyg Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:03.61 +38:29:55.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:03.61 +38:29:55.7: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:03.61 +38:29:55.7: 14.29 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.09 21:28:12.79 +36:49:25.2
83.85759 -10.19015 galactic Cyg Second-epoch detections are separated by 4.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:12.79 +36:49:25.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:12.79 +36:49:25.2: 12.30 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:12.79 +36:49:25.2: 13.57 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 21:55:53.68 +42:08:36.5
91.49484 -9.76702 galactic Cyg Second-epoch detections are separated by 1.8" and 3.7 pix
The object was found in VSX23" Gaia DR3 1960774002240547712
Type: ROT
# Max. Min./Amp. JD0 Period
16.150 G 16.190 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:53.68 +42:08:36.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:53.68 +42:08:36.5: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960774002240547712,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960774002240547712 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.02 21:31:19.68 +39:08:30.9
85.94016 -8.95165 galactic Cyg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was found in VSX 7" Gaia DR3 1964393972479822592
Type: ROT
# Max. Min./Amp. JD0 Period
14.510 G 14.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:19.68 +39:08:30.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:19.68 +39:08:30.9: 13.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1964393972479822592,2461185.8480,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964393972479822592 20260525.3480 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.10 21:51:41.99 +34:07:03.5
85.59063 -15.41687 galactic Peg Second-epoch detections are separated by 4.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:41.99 +34:07:03.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:41.99 +34:07:03.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:41.99 +34:07:03.5: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.19 21:44:02.27 +38:24:38.7
87.29124 -11.16535 galactic Cyg Second-epoch detections are separated by 1.2" and 3.9 pix
The object was found in VSX19" ZTF J214402.43+382419.3
Type: BY
# Max. Min./Amp. JD0 Period
14.839 g Y 0.193 g 2458272.81040 4.094850000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:02.27 +38:24:38.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:02.27 +38:24:38.7: 14.32 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214402.43+382419.3,2461185.8480,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214402.43+382419.3 20260525.3480 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 21:43:24.81 +37:27:40.2
86.55442 -11.79421 galactic Cyg Second-epoch detections are separated by 2.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8421+37.4582 | 21:43:24.81 +37:27:40.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.764+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:24.81 +37:27:40.2: 13.31 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:24.81 +37:27:40.2: 13.79 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8421+37.4582,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8421+37.4582 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 21:41:57.73 +41:24:19.5
89.00099 -8.65732 galactic Cyg Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4872+41.4174 | 21:41:57.73 +41:24:19.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.847+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:57.73 +41:24:19.5: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:57.73 +41:24:19.5: 14.13 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4872+41.4174,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4872+41.4174 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.14 21:42:33.81 +41:45:50.4
89.32610 -8.46272 galactic Cyg Second-epoch detections are separated by 2.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:33.81 +41:45:50.4 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:33.81 +41:45:50.4: 12.96 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:33.81 +41:45:50.4: 14.17 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.13 22:07:12.31 +41:10:46.1
92.59574 -11.82172 galactic Lac Second-epoch detections are separated by 1.1" and 3.3 pix
The object was found in VSX23" Gaia DR3 1956783698448157440
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.680 G 16.770 G 0.047949100000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:12.31 +41:10:46.1: 13.56 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:12.31 +41:10:46.1: 14.60 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956783698448157440,2461185.8480,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956783698448157440 20260525.3480 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.03 21:29:22.39 +34:26:40.6
82.32778 -12.05090 galactic Cyg Second-epoch detections are separated by 1.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:22.39 +34:26:40.6 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:22.39 +34:26:40.6: 13.17 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:22.39 +34:26:40.6: 14.06 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.08 21:32:31.05 +37:13:03.8
84.76361 -10.50487 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952091085897468288 | 21:32:31.02 +37:13:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.594+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:31.05 +37:13:03.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:31.05 +37:13:03.8: 13.58 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952091085897468288,2461185.8480,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952091085897468288 20260525.3480 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 22:09:10.52 +33:47:36.6
88.31348 -17.95342 galactic Peg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:10.52 +33:47:36.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:10.52 +33:47:36.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:10.52 +33:47:36.6: 14.65 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.17 22:03:26.52 +35:25:29.3
88.38674 -15.94154 galactic Peg Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:26.52 +35:25:29.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:26.52 +35:25:29.3: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:26.52 +35:25:29.3: 13.76 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.14 21:41:45.31 +37:40:53.2
86.45436 -11.41095 galactic Cyg Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4361+37.6851 | 21:41:45.31 +37:40:53.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.660+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:45.31 +37:40:53.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:45.31 +37:40:53.2: 14.48 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4361+37.6851,2461185.8480,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4361+37.6851 20260525.3480 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.04 21:29:18.14 +33:38:40.5
81.74123 -12.60939 galactic Cyg Second-epoch detections are separated by 1.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:18.14 +33:38:40.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:18.14 +33:38:40.5: 12.43 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:18.14 +33:38:40.5: 14.23 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.97 22:08:01.57 +35:58:26.1
89.50197 -16.07770 galactic Lac Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9939+35.9764 | 22:08:01.57 +35:58:26.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:01.57 +35:58:26.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:01.57 +35:58:26.1: 13.96 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9939+35.9764,2461185.8480,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9939+35.9764 20260525.3480 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 22:00:45.78 +42:12:40.6
92.25644 -10.27260 galactic Lac Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.1869+42.2151 | 22:00:45.78 +42:12:40.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.575+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:45.78 +42:12:40.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:45.78 +42:12:40.6: 13.86 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1869+42.2151,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1869+42.2151 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.93 21:44:03.17 +37:47:35.8
86.87628 -11.62991 galactic Cyg Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:03.17 +37:47:35.8 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:03.17 +37:47:35.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:03.17 +37:47:35.8: 13.56 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.03 21:57:12.31 +36:23:41.2
87.99601 -14.39450 galactic Peg Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2982+36.3906 | 21:57:11.61 +36:24:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:12.31 +36:23:41.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:12.31 +36:23:41.2: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2982+36.3906,2461185.8480,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2982+36.3906 20260525.3480 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.91 21:49:03.73 +39:29:38.9
88.76636 -10.98614 galactic Cyg Second-epoch detections are separated by 1.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.2650+39.4941 | 21:49:03.73 +39:29:38.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.562+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:03.73 +39:29:38.9: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:03.73 +39:29:38.9: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.2650+39.4941,2461185.8480,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.2650+39.4941 20260525.3480 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 22:03:46.20 +38:55:41.6
90.66622 -13.21893 galactic Lac Second-epoch detections are separated by 2.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:46.20 +38:55:41.6 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:46.20 +38:55:41.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:46.20 +38:55:41.6: 14.25 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.05 21:53:48.08 +40:18:26.1
90.00785 -10.94473 galactic Cyg Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:48.08 +40:18:26.1 (user input) | T | P | (position from user input) J-Ks=0.983+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:48.08 +40:18:26.1: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:48.08 +40:18:26.1: 13.81 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.01 21:45:02.97 +36:40:08.0
86.26610 -12.60341 galactic Cyg Second-epoch detections are separated by 1.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:02.97 +36:40:08.0 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:02.97 +36:40:08.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:02.97 +36:40:08.0: 13.87 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.06 22:08:21.44 +34:16:43.6
88.48251 -17.46528 galactic Peg Second-epoch detections are separated by 1.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:21.44 +34:16:43.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:21.44 +34:16:43.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:21.44 +34:16:43.6: 14.30 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.05 21:34:49.80 +42:03:15.4
88.44352 -7.28371 galactic Cyg Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:49.80 +42:03:15.4 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:49.80 +42:03:15.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:49.80 +42:03:15.4: 13.73 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 21:47:46.78 +37:36:30.0
87.31883 -12.25455 galactic Cyg Second-epoch detections are separated by 1.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952583598387478272 | 21:47:44.78 +37:36:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.291+/-0.050 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:46.78 +37:36:30.0: 13.52 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:46.78 +37:36:30.0: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952583598387478272,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952583598387478272 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.86 21:29:00.32 +38:59:30.2
85.50593 -8.74739 galactic Cyg Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1964564358128327936 | 21:29:00.32 +38:59:30.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.358+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:00.32 +38:59:30.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:00.32 +38:59:30.2: 13.46 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1964564358128327936,2461185.8480,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1964564358128327936 20260525.3480 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.71 21:35:25.71 +40:25:30.5
87.41013 -8.55617 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.8696+40.4280 | 21:35:25.71 +40:25:30.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.667+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:25.71 +40:25:30.5: 11.73 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:25.71 +40:25:30.5: 13.32 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8696+40.4280,2461185.8480,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8696+40.4280 20260525.3480 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.91 21:27:28.02 +39:54:38.6
85.93811 -7.88144 galactic Cyg Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.8597+39.9073 | 21:27:28.02 +39:54:38.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:28.02 +39:54:38.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:28.02 +39:54:38.6: 13.76 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.8597+39.9073,2461185.8480,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8597+39.9073 20260525.3480 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.87 21:53:31.10 +33:46:49.4
85.66044 -15.91831 galactic Peg Second-epoch detections are separated by 1.8" and 3.7 pix
The object was found in VSX17" Gaia DR3 1948095842897373440
Type: E+ROT
# Max. Min./Amp. JD0 Period
15.750 G 15.920 G 1.253330000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:31.10 +33:46:49.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:31.10 +33:46:49.4: 14.21 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948095842897373440,2461185.8480,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948095842897373440 20260525.3480 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.87 21:50:38.82 +39:20:18.3
88.90205 -11.30271 galactic Cyg Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.6717+39.3478 | 21:50:41.21 +39:20:52.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:38.82 +39:20:18.3: 13.61 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:38.82 +39:20:18.3: 14.05 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.6717+39.3478,2461185.8480,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.6717+39.3478 20260525.3480 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.04 21:46:35.91 +37:00:51.7
86.73830 -12.54865 galactic Cyg Second-epoch detections are separated by 2.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:35.91 +37:00:51.7 (user input) | T | P | (position from user input) J-Ks=0.544+/-0.050 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:35.91 +37:00:51.7: 11.99 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:35.91 +37:00:51.7: 13.65 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.75 21:28:06.42 +33:41:27.0
81.59404 -12.40119 galactic Cyg Second-epoch detections are separated by 3.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0376+33.6940 | 21:28:06.42 +33:41:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.486+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:06.42 +33:41:27.0: 12.09 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:06.42 +33:41:27.0: 13.94 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0376+33.6940,2461185.8480,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0376+33.6940 20260525.3480 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 22:07:48.92 +34:48:03.5
88.72297 -16.98320 galactic Peg Second-epoch detections are separated by 1.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:48.92 +34:48:03.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:48.92 +34:48:03.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:48.92 +34:48:03.5: 14.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.95 22:05:32.49 +38:58:33.0
90.97688 -13.39066 galactic Lac Second-epoch detections are separated by 2.0" and 3.4 pix
The object was found in VSX 3" Gaia DR3 1955944191256830592
Type: ROT
# Max. Min./Amp. JD0 Period
14.100 G 14.150 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:32.49 +38:58:33.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:32.49 +38:58:33.0: 13.85 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955944191256830592,2461185.8480,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955944191256830592 20260525.3480 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.88 21:51:31.60 +37:29:39.0
87.82121 -12.82384 galactic Cyg Second-epoch detections are separated by 2.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.8782+37.4956 | 21:51:31.60 +37:29:39.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-0.041 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:31.60 +37:29:39.0: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:31.60 +37:29:39.0: 13.94 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.8782+37.4956,2461185.8480,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.8782+37.4956 20260525.3480 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.95 21:50:30.82 +36:49:51.1
87.22276 -13.19896 galactic Cyg Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:30.82 +36:49:51.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:30.82 +36:49:51.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:30.82 +36:49:51.1: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.91 22:00:16.07 +41:05:52.9
91.48595 -11.09397 galactic Lac Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:16.07 +41:05:52.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:16.07 +41:05:52.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:16.07 +41:05:52.9: 13.97 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.88 21:29:46.34 +35:53:26.3
83.42133 -11.07629 galactic Cyg Second-epoch detections are separated by 3.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:46.34 +35:53:26.3 (user input) | T | P | (position from user input) J-Ks=0.451+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:46.34 +35:53:26.3: 12.60 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:46.34 +35:53:26.3: 13.86 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.90 21:57:31.30 +38:48:28.0
89.60995 -12.56053 galactic Cyg Second-epoch detections are separated by 0.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3824+38.7999 | 21:57:31.30 +38:48:28.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:31.30 +38:48:28.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:31.30 +38:48:28.0: 14.49 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3824+38.7999,2461185.8480,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3824+38.7999 20260525.3480 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.81 21:44:09.01 +35:27:53.6
85.30527 -13.38195 galactic Cyg Second-epoch detections are separated by 2.5" and 4.1 pix
The object was found in VSX17" Gaia DR3 1947797840888788352
Type: ROT
# Max. Min./Amp. JD0 Period
12.820 G 12.850 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:09.01 +35:27:53.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:09.01 +35:27:53.6: 13.34 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947797840888788352,2461185.8480,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947797840888788352 20260525.3480 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.90 21:43:02.34 +34:00:48.1
84.12916 -14.30663 galactic Cyg Second-epoch detections are separated by 1.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947542582391081344 | 21:43:00.64 +34:00:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:02.34 +34:00:48.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:02.34 +34:00:48.1: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947542582391081344,2461185.8480,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947542582391081344 20260525.3480 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.87 21:32:45.10 +38:02:03.6
85.37006 -9.94557 galactic Cyg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:45.10 +38:02:03.6 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:45.10 +38:02:03.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:45.10 +38:02:03.6: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.07 21:51:29.81 +37:52:05.2
88.06374 -12.53422 galactic Cyg Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.8766+37.8680 | 21:51:28.09 +37:51:53.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:29.81 +37:52:05.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:29.81 +37:52:05.2: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.8766+37.8680,2461185.8480,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.8766+37.8680 20260525.3480 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.87 21:42:51.49 +37:11:24.5
86.28584 -11.92289 galactic Cyg Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:51.49 +37:11:24.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.750+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:51.49 +37:11:24.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:51.49 +37:11:24.5: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.77 22:02:54.23 +40:52:40.1
91.74924 -11.57283 galactic Lac Second-epoch detections are separated by 1.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.7317+40.8658 | 22:02:54.23 +40:52:40.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.383+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:54.23 +40:52:40.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:54.23 +40:52:40.1: 14.10 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.7317+40.8658,2461185.8480,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.7317+40.8658 20260525.3480 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.88 21:42:39.00 +37:00:24.2
86.12913 -12.03181 galactic Cyg Second-epoch detections are separated by 7.4" and 4.6 pix
The object was found in VSX18" ASASSN-V J214237.54+370020.4
Type: SR
# Max. Min./Amp. JD0 Period
12.900 V 13.520 V 2458237.38110 59.029051000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:39.00 +37:00:24.2: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:39.00 +37:00:24.2: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214237.54+370020.4,2461185.8480,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214237.54+370020.4 20260525.3480 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.81 22:08:57.22 +36:50:52.7
90.20482 -15.49343 galactic Lac Second-epoch detections are separated by 0.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2395+36.8572 | 22:08:57.22 +36:50:52.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:57.22 +36:50:52.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:57.22 +36:50:52.7: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2395+36.8572,2461185.8480,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2395+36.8572 20260525.3480 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.76 21:40:15.60 +37:50:20.1
86.33833 -11.09603 galactic Cyg Second-epoch detections are separated by 1.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0657+37.8384 | 21:40:15.60 +37:50:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:15.60 +37:50:20.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:15.60 +37:50:20.1: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0657+37.8384,2461185.8480,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0657+37.8384 20260525.3480 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.83 22:07:52.46 +41:59:46.9
93.19489 -11.24006 galactic Lac Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9600+41.9876 | 22:07:52.46 +41:59:46.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.498+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:52.46 +41:59:46.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:52.46 +41:59:46.9: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9600+41.9876,2461185.8480,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9600+41.9876 20260525.3480 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.79 22:10:57.04 +37:02:43.5
90.65925 -15.57397 galactic Lac Second-epoch detections are separated by 2.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:57.04 +37:02:43.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:57.04 +37:02:43.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:57.04 +37:02:43.5: 14.06 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.71 22:06:24.16 +38:41:47.2
90.94035 -13.71457 galactic Lac Second-epoch detections are separated by 3.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.6030+38.6999 | 22:06:24.16 +38:41:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:24.16 +38:41:47.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:24.16 +38:41:47.2: 13.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.6030+38.6999,2461185.8480,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.6030+38.6999 20260525.3480 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.76 21:26:26.98 +37:43:49.9
84.25009 -9.29806 galactic Cyg Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:26:26.98 +37:43:49.9 (user input) | T | P | (position from user input) J-Ks=1.029+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:26.98 +37:43:49.9: 12.79 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:26.98 +37:43:49.9: 13.56 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.78 21:40:39.67 +36:27:52.9
85.45511 -12.16679 galactic Cyg Second-epoch detections are separated by 1.3" and 3.6 pix
The object was found in VSX25" Gaia DR3 1951099846104858240
Type: ROT
# Max. Min./Amp. JD0 Period
14.420 G 14.450 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:39.67 +36:27:52.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:39.67 +36:27:52.9: 13.94 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951099846104858240,2461185.8480,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951099846104858240 20260525.3480 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.69 21:55:19.69 +36:41:47.8
87.89346 -13.92191 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949620242749602432 | 21:55:19.44 +36:42:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:19.69 +36:41:47.8: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:19.69 +36:41:47.8: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949620242749602432,2461185.8480,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949620242749602432 20260525.3480 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.75 21:26:40.74 +39:52:49.0
85.80753 -7.79755 galactic Cyg Second-epoch detections are separated by 1.7" and 3.4 pix
The object was found in VSX24" ASASSN-V J212642.65+395259.2
Type: SR
# Max. Min./Amp. JD0 Period
12.950 V 13.140 V 2457195.02700 33.370000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:40.74 +39:52:49.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:40.74 +39:52:49.0: 13.73 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212642.65+395259.2,2461185.8480,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212642.65+395259.2 20260525.3480 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.67 21:43:23.84 +33:45:14.5
84.00585 -14.54855 galactic Cyg Second-epoch detections are separated by 2.4" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:23.84 +33:45:14.5 (user input) | T | P | (position from user input) J-Ks=0.749+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:23.84 +33:45:14.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:23.84 +33:45:14.5: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.72 21:43:17.63 +38:29:48.8
87.23824 -11.00432 galactic Cyg Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8236+38.4970 | 21:43:17.63 +38:29:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.680+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:17.63 +38:29:48.8: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:17.63 +38:29:48.8: 13.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8236+38.4970,2461185.8480,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8236+38.4970 20260525.3480 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.86 22:03:38.17 +36:16:08.0
88.96057 -15.30230 galactic Peg Second-epoch detections are separated by 2.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:38.17 +36:16:08.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:38.17 +36:16:08.0: 12.12 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:38.17 +36:16:08.0: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.80 21:58:28.78 +40:10:17.0
90.62897 -11.61145 galactic Lac Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6214+40.1726 | 21:58:28.78 +40:10:17.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.423+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:28.78 +40:10:17.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:28.78 +40:10:17.0: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6214+40.1726,2461185.8480,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6214+40.1726 20260525.3480 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.56 21:57:14.45 +42:01:03.9
91.61322 -10.02118 galactic Cyg Second-epoch detections are separated by 0.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.3064+42.0125 | 21:57:14.45 +42:01:03.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.753+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:14.45 +42:01:03.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:14.45 +42:01:03.9: 13.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3064+42.0125,2461185.8480,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3064+42.0125 20260525.3480 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.72 21:33:10.28 +41:39:56.3
87.94869 -7.35806 galactic Cyg Second-epoch detections are separated by 4.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:10.28 +41:39:56.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:10.28 +41:39:56.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:10.28 +41:39:56.3: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.49 21:28:22.15 +41:32:00.3
87.20098 -6.83563 galactic Cyg Second-epoch detections are separated by 4.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0893+41.5337 | 21:28:22.15 +41:32:00.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:22.15 +41:32:00.3: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:22.15 +41:32:00.3: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0893+41.5337,2461185.8480,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0893+41.5337 20260525.3480 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.71 21:29:16.83 +34:43:07.0
82.51057 -11.84243 galactic Cyg Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:16.83 +34:43:07.0 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:16.83 +34:43:07.0: 12.04 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:16.83 +34:43:07.0: 13.62 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.74 22:04:23.77 +39:34:05.5
91.16506 -12.78533 galactic Lac Second-epoch detections are separated by 1.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956534040584630272 | 22:04:23.45 +39:33:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:23.77 +39:34:05.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:23.77 +39:34:05.5: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956534040584630272,2461185.8480,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956534040584630272 20260525.3480 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.77 22:05:37.45 +38:57:41.0
90.98103 -13.41189 galactic Lac Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:37.45 +38:57:41.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:37.45 +38:57:41.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:37.45 +38:57:41.0: 13.75 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.71 21:54:38.60 +36:53:53.5
87.91716 -13.67922 galactic Cyg Second-epoch detections are separated by 1.2" and 3.8 pix
The object was found in VSX 3" Gaia DR3 1949813864175891072
Type: ROT
# Max. Min./Amp. JD0 Period
14.220 G 14.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:38.60 +36:53:53.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:38.60 +36:53:53.5: 13.65 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949813864175891072,2461185.8480,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949813864175891072 20260525.3480 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.34 21:30:29.91 +39:49:30.6
86.30064 -8.34713 galactic Cyg Second-epoch detections are separated by 1.5" and 3.3 pix
The object was found in VSX19" Gaia DR3 1966123744785952000
Type: ROT
# Max. Min./Amp. JD0 Period
15.950 G 15.980 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:29.91 +39:49:30.6: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:29.91 +39:49:30.6: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966123744785952000,2461185.8480,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966123744785952000 20260525.3480 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.54 21:48:12.58 +41:41:12.5
90.08208 -9.20957 galactic Cyg Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960503900338500992 | 21:48:14.24 +41:40:60.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.489+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:12.58 +41:41:12.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:12.58 +41:41:12.5: 13.26 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960503900338500992,2461185.8480,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960503900338500992 20260525.3480 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.63 21:30:08.27 +37:30:28.0
84.62152 -9.96807 galactic Cyg Second-epoch detections are separated by 3.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.5413+37.5123 | 21:30:08.27 +37:30:28.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.669+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:08.27 +37:30:28.0: 11.63 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:08.27 +37:30:28.0: 13.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.5413+37.5123,2461185.8480,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.5413+37.5123 20260525.3480 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.40 21:45:30.14 +42:12:25.2
90.03664 -8.48707 galactic Cyg Second-epoch detections are separated by 1.8" and 3.3 pix
The object was found in VSX16" Gaia DR3 1972591037821053952
Type: ROT
# Max. Min./Amp. JD0 Period
15.340 G 15.380 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:30.14 +42:12:25.2: 11.47 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:30.14 +42:12:25.2: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972591037821053952,2461185.8480,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972591037821053952 20260525.3480 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.46 22:03:06.42 +40:42:37.9
91.67630 -11.72889 galactic Lac Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:06.42 +40:42:37.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.274+/-0.034 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:06.42 +40:42:37.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:06.42 +40:42:37.9: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.60 21:44:13.05 +38:35:36.7
87.44131 -11.05152 galactic Cyg Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953622331937116928 | 21:44:13.81 +38:34:51.7 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:13.05 +38:35:36.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:13.05 +38:35:36.7: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953622331937116928,2461185.8480,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953622331937116928 20260525.3480 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.52 21:58:00.76 +37:39:30.9
88.94630 -13.51548 galactic Lac Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:00.76 +37:39:30.9 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:00.76 +37:39:30.9: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:00.76 +37:39:30.9: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.44 21:28:31.47 +41:22:58.2
87.11678 -6.96422 galactic Cyg Second-epoch detections are separated by 4.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.1297+41.3819 | 21:28:31.47 +41:22:58.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:31.47 +41:22:58.2: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:31.47 +41:22:58.2: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.1297+41.3819,2461185.8480,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.1297+41.3819 20260525.3480 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.34 21:31:31.11 +41:31:49.7
87.62838 -7.24485 galactic Cyg Second-epoch detections are separated by 2.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8877+41.5332 | 21:31:33.07 +41:31:59.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.450+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:31.11 +41:31:49.7: 13.07 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:31.11 +41:31:49.7: 13.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.8877+41.5332,2461185.8480,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.8877+41.5332 20260525.3480 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.35 22:01:22.48 +40:55:08.5
91.54165 -11.36352 galactic Lac Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3389+40.9153 | 22:01:22.48 +40:55:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.776+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.48 +40:55:08.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:22.48 +40:55:08.5: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3389+40.9153,2461185.8480,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3389+40.9153 20260525.3480 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.37 21:40:43.84 +37:22:59.4
86.09661 -11.49628 galactic Cyg Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1759+37.3947 | 21:40:43.84 +37:22:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.217+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:43.84 +37:22:59.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:43.84 +37:22:59.4: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1759+37.3947,2461185.8480,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1759+37.3947 20260525.3480 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.27 21:40:26.40 +39:27:29.0
87.46865 -9.91799 galactic Cyg Second-epoch detections are separated by 1.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:26.40 +39:27:29.0 (user input) | T | P | (position from user input) J-Ks=0.997+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:26.40 +39:27:29.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:26.40 +39:27:29.0: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.21 21:33:11.14 +39:46:10.4
86.64050 -8.74278 galactic Cyg Second-epoch detections are separated by 1.1" and 3.5 pix
The object was found in VSX11" NSVS 5918143
Type: SR
# Max. Min./Amp. JD0 Period
13.055 r Y 0.513 r 2458273.93180 220.436025900000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:11.14 +39:46:10.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:11.14 +39:46:10.4: 13.34 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5918143,2461185.8480,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5918143 20260525.3480 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.25 22:02:11.40 +35:32:41.6
88.25655 -15.68917 galactic Peg Second-epoch detections are separated by 0.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948505887717109376 | 22:02:11.25 +35:33:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:11.40 +35:32:41.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:11.40 +35:32:41.6: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948505887717109376,2461185.8480,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948505887717109376 20260525.3480 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.37 21:49:22.29 +41:57:46.4
90.42999 -9.13810 galactic Cyg Second-epoch detections are separated by 2.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:22.29 +41:57:46.4 (user input) | T | P | (position from user input) J-Ks=0.687+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:22.29 +41:57:46.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:22.29 +41:57:46.4: 12.98 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.25 21:57:39.33 +41:47:18.3
91.52959 -10.24871 galactic Lac Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.4174+41.7911 | 21:57:39.33 +41:47:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.534+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:39.33 +41:47:18.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.33 +41:47:18.3: 13.46 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4174+41.7911,2461185.8480,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4174+41.7911 20260525.3480 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.30 21:50:25.17 +35:00:16.6
85.98309 -14.57278 galactic Peg Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.6155+34.9987 | 21:50:25.17 +35:00:16.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:25.17 +35:00:16.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:25.17 +35:00:16.6: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.6155+34.9987,2461185.8480,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.6155+34.9987 20260525.3480 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.04 21:30:28.13 +38:52:35.3
85.63224 -9.02794 galactic Cyg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.6201+38.8826 | 21:30:28.13 +38:52:35.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.702+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:28.13 +38:52:35.3: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:28.13 +38:52:35.3: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.6201+38.8826,2461185.8480,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.6201+38.8826 20260525.3480 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.10 21:35:35.36 +35:59:26.5
84.35874 -11.81935 galactic Cyg Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951030748672306944 | 21:35:37.59 +35:59:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.355+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:35.36 +35:59:26.5: 12.85 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:35.36 +35:59:26.5: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951030748672306944,2461185.8480,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951030748672306944 20260525.3480 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.03 21:34:37.63 +34:15:56.3
82.99662 -12.93490 galactic Cyg Second-epoch detections are separated by 0.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:37.63 +34:15:56.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:37.63 +34:15:56.3: 13.17 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:37.63 +34:15:56.3: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.15 22:10:32.03 +41:45:05.9
93.45513 -11.72990 galactic Lac Second-epoch detections are separated by 1.3" and 3.4 pix
The object was found in VSX 1" Gaia DR3 1958278935478930816
Type: ROT
# Max. Min./Amp. JD0 Period
13.370 G 13.410 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:32.03 +41:45:05.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:32.03 +41:45:05.9: 13.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958278935478930816,2461185.8480,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958278935478930816 20260525.3480 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.05 22:11:02.23 +38:11:05.6
91.37461 -14.66745 galactic Lac Second-epoch detections are separated by 0.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955415905978584576 | 22:11:03.83 +38:11:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.358+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:02.23 +38:11:05.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:02.23 +38:11:05.6: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955415905978584576,2461185.8480,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955415905978584576 20260525.3480 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.02 22:12:04.92 +39:17:50.0
92.22150 -13.88950 galactic Lac Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955621725110826496 | 22:12:03.02 +39:17:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:04.92 +39:17:50.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:04.92 +39:17:50.0: 99.00 +/- 99.00 bad_region
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955621725110826496,2461185.8480,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955621725110826496 20260525.3480 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.04 21:40:56.14 +41:13:20.7
88.73229 -8.66627 galactic Cyg Second-epoch detections are separated by 1.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2343+41.2229 | 21:40:56.14 +41:13:20.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.331+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:56.14 +41:13:20.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:56.14 +41:13:20.7: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2343+41.2229,2461185.8480,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2343+41.2229 20260525.3480 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.97 22:07:02.72 +41:57:30.8
93.04573 -11.17874 galactic Lac Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.7672+41.9608 | 22:07:02.72 +41:57:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:02.72 +41:57:30.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:02.72 +41:57:30.8: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.7672+41.9608,2461185.8480,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.7672+41.9608 20260525.3480 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.89 21:44:09.61 +37:55:02.7
86.97645 -11.55098 galactic Cyg Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.0405+37.9120 | 21:44:11.54 +37:55:07.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.406+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:09.61 +37:55:02.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:09.61 +37:55:02.7: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.0405+37.9120,2461185.8480,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.0405+37.9120 20260525.3480 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.78 21:33:22.18 +38:02:28.7
85.46458 -10.02425 galactic Cyg Second-epoch detections are separated by 1.3" and 3.8 pix
The object was found in VSX19" V1615 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.200 pg < 17.500 pg 2442995.00000 268.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:22.18 +38:02:28.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:22.18 +38:02:28.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1615 Cyg,2461185.8480,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1615 Cyg 20260525.3480 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.95 22:05:39.89 +34:53:38.5
88.41798 -16.63956 galactic Peg Second-epoch detections are separated by 0.4" and 3.7 pix
The object was found in VSX20" Gaia DR3 1900468744392395008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.160 G 13.190 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:39.89 +34:53:38.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:39.89 +34:53:38.5: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1900468744392395008,2461185.8480,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1900468744392395008 20260525.3480 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.75 21:33:13.81 +37:12:44.0
84.86424 -10.60674 galactic Cyg Second-epoch detections are separated by 1.0" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952077135843691520 | 21:33:13.84 +37:13:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.344+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:13.81 +37:12:44.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:13.81 +37:12:44.0: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952077135843691520,2461185.8480,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952077135843691520 20260525.3480 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.77 21:59:20.91 +36:56:49.2
88.69948 -14.23625 galactic Lac Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:20.91 +36:56:49.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.647+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:20.91 +36:56:49.2: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:20.91 +36:56:49.2: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.80 22:06:30.62 +34:18:24.6
88.18433 -17.20974 galactic Peg Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:30.62 +34:18:24.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:30.62 +34:18:24.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:30.62 +34:18:24.6: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.84 21:59:59.23 +36:08:33.3
88.28201 -14.94358 galactic Peg Second-epoch detections are separated by 1.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9994+36.1363 | 21:59:59.86 +36:08:10.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:59.23 +36:08:33.3: 12.02 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:59.23 +36:08:33.3: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9994+36.1363,2461185.8480,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9994+36.1363 20260525.3480 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.70 21:37:46.88 +36:44:34.4
85.21241 -11.57095 galactic Cyg Second-epoch detections are separated by 1.9" and 3.7 pix
The object was found in VSX24" ASASSN-V J213745.82+364414.6
Type: L
# Max. Min./Amp. JD0 Period
11.610 V 11.730 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:46.88 +36:44:34.4: 13.36 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:46.88 +36:44:34.4: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213745.82+364414.6,2461185.8480,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213745.82+364414.6 20260525.3480 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.61 21:28:09.30 +41:14:37.1
86.96909 -7.01616 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0200+41.2443 | 21:28:07.89 +41:14:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.370+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:09.30 +41:14:37.1: 12.09 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:09.30 +41:14:37.1: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0200+41.2443,2461185.8480,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0200+41.2443 20260525.3480 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.55 21:32:51.76 +35:15:25.9
83.43176 -11.96848 galactic Cyg Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.2165+35.2577 | 21:32:51.76 +35:15:25.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:51.76 +35:15:25.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:51.76 +35:15:25.9: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.2165+35.2577,2461185.8480,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.2165+35.2577 20260525.3480 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.56 21:56:52.31 +39:21:22.0
89.86178 -12.05453 galactic Cyg Second-epoch detections are separated by 1.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2160+39.3666 | 21:56:52.31 +39:21:22.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.795+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:52.31 +39:21:22.0: 12.42 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:52.31 +39:21:22.0: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2160+39.3666,2461185.8480,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2160+39.3666 20260525.3480 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.67 21:27:20.05 +35:46:48.2
82.98370 -10.80834 galactic Cyg Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951517935397882496 | 21:27:20.07 +35:47:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.482+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:20.05 +35:46:48.2: 11.26 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:20.05 +35:46:48.2: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951517935397882496,2461185.8480,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951517935397882496 20260525.3480 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.56 21:28:11.99 +34:45:25.7
82.37701 -11.65892 galactic Cyg Second-epoch detections are separated by 3.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:11.99 +34:45:25.7 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.027 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:11.99 +34:45:25.7: 10.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.99 +34:45:25.7: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.61 21:54:25.08 +39:39:28.0
89.68111 -11.52185 galactic Cyg Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959168337307618304 | 21:54:23.59 +39:39:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.125+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:25.08 +39:39:28.0: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:25.08 +39:39:28.0: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959168337307618304,2461185.8480,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959168337307618304 20260525.3480 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.51 21:30:32.04 +35:46:44.4
83.45453 -11.26399 galactic Cyg Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:32.04 +35:46:44.4 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:32.04 +35:46:44.4: 12.80 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:32.04 +35:46:44.4: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.14 21:46:48.64 +36:53:20.3
86.68645 -12.67096 galactic Cyg Second-epoch detections are separated by 1.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952523748021879296 | 21:46:47.09 +36:53:34.1 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=0.888+/-0.028 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:48.64 +36:53:20.3: 13.63 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:48.64 +36:53:20.3: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952523748021879296,2461185.8480,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952523748021879296 20260525.3480 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.21 21:38:15.46 +38:02:08.4
86.17637 -10.68459 galactic Cyg Second-epoch detections are separated by 1.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5674+38.0416 | 21:38:15.13 +38:02:26.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:15.46 +38:02:08.4: 11.77 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:15.46 +38:02:08.4: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5674+38.0416,2461185.8480,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5674+38.0416 20260525.3480 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.90 21:36:49.67 +39:45:20.6
87.14979 -9.22966 galactic Cyg Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1965969366481229952 | 21:36:48.10 +39:45:16.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.284+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:49.67 +39:45:20.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:49.67 +39:45:20.6: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965969366481229952,2461185.8480,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965969366481229952 20260525.3480 9.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.87 22:06:56.78 +36:48:40.3
89.84975 -15.28012 galactic Lac Second-epoch detections are separated by 0.6" and 3.5 pix
The object was found in VSX 1" ASASSN-V J220656.79+364840.9
Type: SR
# Max. Min./Amp. JD0 Period
12.720 g Y 0.400 g 2458496.54800 580.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:56.78 +36:48:40.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:56.78 +36:48:40.3: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J220656.79+364840.9,2461185.8480,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220656.79+364840.9 20260525.3480 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.78 22:00:17.84 +38:06:34.9
89.59810 -13.44508 galactic Lac Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.0789+38.1088 | 22:00:18.96 +38:06:31.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:17.84 +38:06:34.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:17.84 +38:06:34.9: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.0789+38.1088,2461185.8480,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.0789+38.1088 20260525.3480 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.79 21:59:06.43 +34:00:17.5
86.73709 -16.48980 galactic Peg Second-epoch detections are separated by 0.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1947975824331378048 | 21:59:07.15 +34:00:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:06.43 +34:00:17.5: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:06.43 +34:00:17.5: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947975824331378048,2461185.8480,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947975824331378048 20260525.3480 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.68 22:01:18.69 +41:30:27.6
91.89988 -10.89119 galactic Lac Second-epoch detections are separated by 0.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959759393525967360 | 22:01:19.91 +41:30:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.219+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:18.69 +41:30:27.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:18.69 +41:30:27.6: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959759393525967360,2461185.8480,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959759393525967360 20260525.3480 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.48 21:34:29.38 +39:23:38.8
86.56601 -9.18851 galactic Cyg Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1965875770554661504 | 21:34:28.39 +39:23:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.762+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:29.38 +39:23:38.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:29.38 +39:23:38.8: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965875770554661504,2461185.8480,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965875770554661504 20260525.3480 9.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 8.37 22:01:14.44 +38:33:47.4
90.03615 -13.20390 galactic Lac Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3181+38.5754 | 22:01:16.11 +38:33:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.852+/-0.052 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:14.44 +38:33:47.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:14.44 +38:33:47.4: 10.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.14 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3181+38.5754,2461185.8480,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3181+38.5754 20260525.3480 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 9.59 21:31:14.97 +38:46:29.7
85.67224 -9.20647 galactic Cyg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was found in VSX 3" V2072 Cyg
Type: M
# Max. Min./Amp. JD0 Period
10.400 V 17.900 V 2451388.00000 317.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:14.97 +38:46:29.7: 12.71 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:14.97 +38:46:29.7: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2072 Cyg,2461185.8480,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2072 Cyg 20260525.3480 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.33 22:09:13.59 +39:15:46.5
91.74187 -13.59041 galactic Lac Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956289747146754688 | 22:09:11.61 +39:15:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.504+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:13.59 +39:15:46.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:13.59 +39:15:46.5: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956289747146754688,2461185.8480,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956289747146754688 20260525.3480 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.53 21:44:42.94 +35:29:07.5
85.40758 -13.44337 galactic Cyg Second-epoch detections are separated by 0.4" and 3.8 pix
The object was found in VSX 0" ASASSN-V J214442.97+352907.2
Type: SR
# Max. Min./Amp. JD0 Period
14.180 g Y 0.300 g 2458641.96400 41.070000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:42.94 +35:29:07.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:42.94 +35:29:07.5: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214442.97+352907.2,2461185.8480,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214442.97+352907.2 20260525.3480 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.79 22:02:13.94 +41:47:07.6
92.21136 -10.77648 galactic Lac Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5515+41.7805 | 22:02:12.37 +41:46:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.975+/-0.036 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:13.94 +41:47:07.6: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:13.94 +41:47:07.6: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5515+41.7805,2461185.8480,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5515+41.7805 20260525.3480 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.72 21:43:06.26 +37:12:23.6
86.33438 -11.94333 galactic Cyg Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:06.26 +37:12:23.6 (user input) | T | P | (position from user input) J-Ks=0.793+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:06.26 +37:12:23.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:06.26 +37:12:23.6: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.93 21:40:41.05 +36:19:20.5
85.36054 -12.27512 galactic Cyg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1711+36.3226 | 21:40:38.96 +36:19:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:41.05 +36:19:20.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:41.05 +36:19:20.5: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1711+36.3226,2461185.8480,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1711+36.3226 20260525.3480 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.13 22:02:42.11 +37:08:59.4
89.37057 -14.49351 galactic Lac Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:42.11 +37:08:59.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.11 +37:08:59.4: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.11 +37:08:59.4: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.19 22:02:14.92 +34:37:08.3
87.66573 -16.42067 galactic Peg Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5676+34.6142 | 22:02:14.92 +34:37:08.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:14.92 +34:37:08.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:14.92 +34:37:08.3: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5676+34.6142,2461185.8480,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5676+34.6142 20260525.3480 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.23 22:02:42.57 +41:44:09.7
92.25256 -10.86987 galactic Lac Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959859277284333312 | 22:02:40.01 +41:44:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.57 +41:44:09.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.57 +41:44:09.7: 13.61 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959859277284333312,2461185.8480,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959859277284333312 20260525.3480 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.35 22:00:24.33 +35:58:53.7
88.24586 -15.12204 galactic Peg Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948721361934626432 | 22:00:23.05 +35:59:18.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:24.33 +35:58:53.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:24.33 +35:58:53.7: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948721361934626432,2461185.8480,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948721361934626432 20260525.3480 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.22 22:03:19.33 +33:44:47.9
87.27812 -17.24081 galactic Peg Second-epoch detections are separated by 1.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.8337+33.7460 | 22:03:19.74 +33:44:19.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:19.33 +33:44:47.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:19.33 +33:44:47.9: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.8337+33.7460,2461185.8480,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.8337+33.7460 20260525.3480 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.30 22:10:02.92 +36:44:11.9
90.31757 -15.71402 galactic Lac Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1954722908717995392 | 22:10:01.34 +36:44:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.370+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:02.92 +36:44:11.9: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:02.92 +36:44:11.9: 13.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954722908717995392,2461185.8480,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954722908717995392 20260525.3480 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.29 21:49:08.07 +35:40:21.4
86.22922 -13.89604 galactic Cyg Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.3029+35.6719 | 21:49:10.54 +35:40:10.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.396+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:08.07 +35:40:21.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:08.07 +35:40:21.4: 12.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.3029+35.6719,2461185.8480,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.3029+35.6719 20260525.3480 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.38 22:06:31.92 +34:33:33.0
88.35006 -17.01326 galactic Peg Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:31.92 +34:33:33.0 (user input) | T | P | (position from user input) J-Ks=0.631+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:31.92 +34:33:33.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:31.92 +34:33:33.0: 14.31 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.35 21:54:12.72 +35:10:05.1
86.70356 -14.95129 galactic Peg Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.5434+35.1779 | 21:54:10.46 +35:10:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:12.72 +35:10:05.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:12.72 +35:10:05.1: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.5434+35.1779,2461185.8480,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.5434+35.1779 20260525.3480 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.46 21:40:47.62 +37:32:56.2
86.21960 -11.38180 galactic Cyg Second-epoch detections are separated by 0.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953471527045546752 | 21:40:46.82 +37:33:21.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.770+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:47.62 +37:32:56.2: 12.51 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:47.62 +37:32:56.2: 13.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953471527045546752,2461185.8480,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953471527045546752 20260525.3480 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.54 22:09:46.32 +41:39:59.1
93.28650 -11.71520 galactic Lac Second-epoch detections are separated by 1.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1958254196465679360 | 22:09:49.52 +41:39:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:46.32 +41:39:59.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:46.32 +41:39:59.1: 13.92 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958254196465679360,2461185.8480,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958254196465679360 20260525.3480 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.46 21:47:33.77 +37:22:55.8
87.13399 -12.39736 galactic Cyg Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:33.77 +37:22:55.8 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:33.77 +37:22:55.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:33.77 +37:22:55.8: 13.86 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.46 21:33:58.57 +36:17:17.8
84.32608 -11.37935 galactic Cyg Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J213356.94+361650.1 | 21:33:56.95 +36:16:50.1 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:58.57 +36:17:17.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:58.57 +36:17:17.8: 13.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213356.94+361650.1,2461185.8480,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213356.94+361650.1 20260525.3480 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.52 22:04:59.77 +39:57:17.5
91.49943 -12.54789 galactic Lac Second-epoch detections are separated by 1.1" and 3.6 pix
The object was found in VSX 2" Gaia DR3 1956561223437486208
Type: ROT
# Max. Min./Amp. JD0 Period
13.720 G 13.750 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:59.77 +39:57:17.5: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:59.77 +39:57:17.5: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956561223437486208,2461185.8480,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956561223437486208 20260525.3480 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.44 21:48:15.82 +35:31:04.0
85.98694 -13.89677 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949244592030369792 | 21:48:15.63 +35:31:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.411+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:15.82 +35:31:04.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:15.82 +35:31:04.0: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949244592030369792,2461185.8480,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949244592030369792 20260525.3480 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.55 22:02:04.72 +37:45:26.3
89.65715 -13.93930 galactic Lac Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:04.72 +37:45:26.3 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:04.72 +37:45:26.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:04.72 +37:45:26.3: 14.38 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.63 21:54:39.47 +39:49:48.7
89.82895 -11.41763 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J215437.58+395008.3 | 21:54:37.58 +39:50:08.3 (Gaia DR3) | SR (local) | 2458650.78900 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.749+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:39.47 +39:49:48.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:39.47 +39:49:48.7: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215437.58+395008.3,2461185.8480,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215437.58+395008.3 20260525.3480 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.66 22:11:31.18 +40:27:17.9
92.83025 -12.88883 galactic Lac Second-epoch detections are separated by 1.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956459587331702016 | 22:11:28.70 +40:27:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.161+/-0.053 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:31.18 +40:27:17.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:31.18 +40:27:17.9: 13.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956459587331702016,2461185.8480,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956459587331702016 20260525.3480 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.65 22:05:42.70 +35:53:01.6
89.05834 -15.86383 galactic Lac Second-epoch detections are separated by 2.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.4278+35.8836 | 22:05:42.70 +35:53:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.451+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:42.70 +35:53:01.6: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:42.70 +35:53:01.6: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.4278+35.8836,2461185.8480,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.4278+35.8836 20260525.3480 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.56 21:48:57.95 +37:42:52.3
87.57180 -12.32730 galactic Cyg Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.2399+37.7077 | 21:48:57.59 +37:42:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:57.95 +37:42:52.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:57.95 +37:42:52.3: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.2399+37.7077,2461185.8480,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.2399+37.7077 20260525.3480 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.66 21:58:42.71 +38:46:43.2
89.77664 -12.72838 galactic Lac Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956079568625293952 | 21:58:44.20 +38:47:24.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5) J-Ks=0.324+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:42.71 +38:46:43.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:42.71 +38:46:43.2: 13.97 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956079568625293952,2461185.8480,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956079568625293952 20260525.3480 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.72 22:10:20.20 +38:44:20.8
91.59990 -14.13986 galactic Lac Second-epoch detections are separated by 1.1" and 3.4 pix
The object was found in VSX 1" Gaia DR3 1955512632942240128
Type: ROT
# Max. Min./Amp. JD0 Period
13.880 G 13.920 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:20.20 +38:44:20.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:20.20 +38:44:20.8: 14.41 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955512632942240128,2461185.8480,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955512632942240128 20260525.3480 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.61 21:58:43.33 +42:11:57.9
91.94649 -10.04923 galactic Lac Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6664+42.1926 | 21:58:43.33 +42:11:57.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.761+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:43.33 +42:11:57.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:43.33 +42:11:57.9: 14.03 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6664+42.1926,2461185.8480,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6664+42.1926 20260525.3480 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.71 21:49:41.31 +37:43:29.6
87.68985 -12.41234 galactic Cyg Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.4213+37.7226 | 21:49:42.64 +37:43:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.682+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:41.31 +37:43:29.6: 13.26 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:41.31 +37:43:29.6: 13.64 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.4213+37.7226,2461185.8480,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4213+37.7226 20260525.3480 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.68 21:51:57.64 +37:11:55.0
87.69326 -13.10535 galactic Cyg Second-epoch detections are separated by 0.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949874199877180800 | 21:51:57.22 +37:12:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.432+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:57.64 +37:11:55.0: 12.47 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:57.64 +37:11:55.0: 13.89 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949874199877180800,2461185.8480,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949874199877180800 20260525.3480 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.79 22:06:28.76 +39:03:18.4
91.17533 -13.43764 galactic Lac Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956273907300611968 | 22:06:31.70 +39:03:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:28.76 +39:03:18.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:28.76 +39:03:18.4: 14.01 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956273907300611968,2461185.8480,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956273907300611968 20260525.3480 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.81 22:00:37.00 +35:01:34.4
87.65922 -15.89342 galactic Peg Second-epoch detections are separated by 1.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.1381+35.0359 | 22:00:35.41 +35:02:13.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.847+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:37.00 +35:01:34.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:37.00 +35:01:34.4: 14.35 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1381+35.0359,2461185.8480,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1381+35.0359 20260525.3480 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.62 21:59:40.08 +41:01:41.0
91.35129 -11.07928 galactic Lac Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9159+41.0218 | 21:59:39.84 +41:01:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:40.08 +41:01:41.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:40.08 +41:01:41.0: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9159+41.0218,2461185.8480,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9159+41.0218 20260525.3480 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.80 22:00:24.47 +39:57:06.7
90.78560 -12.01245 galactic Lac Second-epoch detections are separated by 1.0" and 3.4 pix
The object was found in VSX 5" Gaia DR3 1959243104097280768
Type: ROT
# Max. Min./Amp. JD0 Period
15.910 G 15.960 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:24.47 +39:57:06.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:24.47 +39:57:06.7: 13.88 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959243104097280768,2461185.8480,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959243104097280768 20260525.3480 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.75 22:07:43.41 +37:37:06.0
90.48273 -14.73092 galactic Lac Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.9384+37.6117 | 22:07:43.41 +37:37:06.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:43.41 +37:37:06.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:43.41 +37:37:06.0: 14.14 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9384+37.6117,2461185.8480,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9384+37.6117 20260525.3480 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.80 22:01:04.09 +41:04:55.5
91.59714 -11.19929 galactic Lac Second-epoch detections are separated by 2.9" and 3.0 pix
The object was found in VSX 5" Gaia DR3 1959714932024123904
Type: ROT
# Max. Min./Amp. JD0 Period
14.280 G 14.310 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:04.09 +41:04:55.5: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:04.09 +41:04:55.5: 13.90 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959714932024123904,2461185.8480,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959714932024123904 20260525.3480 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.80 22:11:43.30 +42:07:49.5
93.86428 -11.55194 galactic Lac Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:43.30 +42:07:49.5 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:43.30 +42:07:49.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:43.30 +42:07:49.5: 14.33 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.70 21:36:14.22 +40:15:40.1
87.41207 -8.78117 galactic Cyg Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.0750+40.2537 | 21:36:15.96 +40:15:26.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.709+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:14.22 +40:15:40.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:14.22 +40:15:40.1: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.0750+40.2537,2461185.8480,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0750+40.2537 20260525.3480 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.70 21:33:15.00 +33:54:30.0
82.53157 -12.99480 galactic Cyg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J213311.49+335442.1 | 21:33:11.49 +33:54:42.1 (Gaia DR3) | SRS (local) | 22.560000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:15.00 +33:54:30.0: 12.68 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:15.00 +33:54:30.0: 14.07 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213311.49+335442.1,2461185.8480,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213311.49+335442.1 20260525.3480 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.77 21:56:29.42 +36:52:34.4
88.19616 -13.93115 galactic Cyg Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1195+36.8762 | 21:56:29.42 +36:52:34.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:29.42 +36:52:34.4: 12.11 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:29.42 +36:52:34.4: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1195+36.8762,2461185.8480,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1195+36.8762 20260525.3480 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.81 21:59:28.83 +37:59:48.3
89.39643 -13.43331 galactic Lac Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.8746+37.9877 | 21:59:28.83 +37:59:48.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:28.83 +37:59:48.3: 13.62 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:28.83 +37:59:48.3: 14.19 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.8746+37.9877,2461185.8480,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.8746+37.9877 20260525.3480 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.71 21:35:57.86 +41:51:55.7
88.47096 -7.56545 galactic Cyg Second-epoch detections are separated by 1.5" and 3.2 pix
The object was found in VSX13" Gaia DR3 1966751669007044992
Type: ROT
# Max. Min./Amp. JD0 Period
14.850 G 14.880 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:57.86 +41:51:55.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:57.86 +41:51:55.7: 13.82 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966751669007044992,2461185.8480,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966751669007044992 20260525.3480 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.82 22:09:11.66 +36:46:05.4
90.19499 -15.58617 galactic Lac Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2936+36.7689 | 22:09:11.66 +36:46:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.423+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:11.66 +36:46:05.4: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:11.66 +36:46:05.4: 14.83 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2936+36.7689,2461185.8480,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2936+36.7689 20260525.3480 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.73 21:41:04.38 +37:16:08.3
86.06987 -11.62661 galactic Cyg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2513+37.2756 | 21:41:03.22 +37:16:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:04.38 +37:16:08.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:04.38 +37:16:08.3: 13.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2513+37.2756,2461185.8480,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2513+37.2756 20260525.3480 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.79 21:58:52.18 +37:02:33.4
88.68449 -14.10182 galactic Lac Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949670584068913280 | 21:58:49.46 +37:02:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:52.18 +37:02:33.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:52.18 +37:02:33.4: 14.10 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949670584068913280,2461185.8480,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949670584068913280 20260525.3480 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.81 22:09:33.65 +41:54:58.8
93.40440 -11.49010 galactic Lac Second-epoch detections are separated by 1.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:33.65 +41:54:58.8 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:33.65 +41:54:58.8: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:33.65 +41:54:58.8: 14.25 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.79 21:51:03.60 +36:58:53.3
87.40843 -13.15506 galactic Cyg Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949489920563718528 | 21:51:05.53 +36:58:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=0.405+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:03.60 +36:58:53.3: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:03.60 +36:58:53.3: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949489920563718528,2461185.8480,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949489920563718528 20260525.3480 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.02 22:02:20.04 +34:02:55.5
87.30808 -16.87680 galactic Peg Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:20.04 +34:02:55.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:20.04 +34:02:55.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:20.04 +34:02:55.5: 14.30 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.79 21:47:12.13 +36:46:39.3
86.67187 -12.80639 galactic Cyg Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952472135393923456 | 21:47:13.44 +36:46:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.667+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:12.13 +36:46:39.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:12.13 +36:46:39.3: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952472135393923456,2461185.8480,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952472135393923456 20260525.3480 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.84 21:55:27.21 +41:39:30.1
91.12114 -10.09348 galactic Cyg Second-epoch detections are separated by 2.6" and 3.5 pix
The object was found in VSX22" ASASSN-V J215527.65+413951.1
Type: RRAB
# Max. Min./Amp. JD0 Period
14.640 V 15.050 V 2457989.96900 0.382087000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:27.21 +41:39:30.1: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:27.21 +41:39:30.1: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J215527.65+413951.1,2461185.8480,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215527.65+413951.1 20260525.3480 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.84 21:46:37.68 +36:31:34.8
86.41332 -12.91977 galactic Cyg Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952372805691560064 | 21:46:39.44 +36:31:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.636+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:37.68 +36:31:34.8: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:37.68 +36:31:34.8: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952372805691560064,2461185.8480,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952372805691560064 20260525.3480 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.93 22:01:20.19 +41:45:32.7
92.06038 -10.69530 galactic Lac Second-epoch detections are separated by 2.2" and 3.5 pix
The object was found in VSX23" Gaia DR3 1959956068669176064
Type: ROT
# Max. Min./Amp. JD0 Period
16.640 G 16.700 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:20.19 +41:45:32.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:20.19 +41:45:32.7: 13.91 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959956068669176064,2461185.8480,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959956068669176064 20260525.3480 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.87 21:57:35.09 +40:21:27.2
90.61121 -11.35947 galactic Cyg Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959305054704973056 | 21:57:34.24 +40:21:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:35.09 +40:21:27.2: 12.74 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:35.09 +40:21:27.2: 13.73 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959305054704973056,2461185.8480,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959305054704973056 20260525.3480 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.86 21:48:08.00 +39:26:18.8
88.59070 -10.91211 galactic Cyg Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.0163+39.4455 | 21:48:06.78 +39:26:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:08.00 +39:26:18.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:08.00 +39:26:18.8: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.0163+39.4455,2461185.8480,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.0163+39.4455 20260525.3480 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.91 21:59:05.04 +35:36:42.6
87.78918 -15.24149 galactic Peg Second-epoch detections are separated by 2.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:05.04 +35:36:42.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:05.04 +35:36:42.6: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:05.04 +35:36:42.6: 14.37 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.88 21:50:41.80 +36:02:33.6
86.72497 -13.82213 galactic Peg Second-epoch detections are separated by 0.5" and 3.8 pix
The object was found in VSX21" Gaia DR3 1949369524038765824
Type: ROT
# Max. Min./Amp. JD0 Period
15.990 G 16.010 G 0.349654000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:41.80 +36:02:33.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:41.80 +36:02:33.6: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949369524038765824,2461185.8480,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949369524038765824 20260525.3480 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.88 22:04:54.69 +35:49:32.1
88.88813 -15.81034 galactic Peg Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.2245+35.8493 | 22:04:53.90 +35:50:15.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:54.69 +35:49:32.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:54.69 +35:49:32.1: 14.11 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.2245+35.8493,2461185.8480,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2245+35.8493 20260525.3480 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.85 22:09:59.93 +38:20:08.0
91.29762 -14.42518 galactic Lac Second-epoch detections are separated by 4.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.5078+38.3362 | 22:09:59.93 +38:20:08.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:59.93 +38:20:08.0: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:59.93 +38:20:08.0: 14.38 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.5078+38.3362,2461185.8480,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.5078+38.3362 20260525.3480 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.76 21:27:56.81 +35:27:16.8
82.84043 -11.12709 galactic Cyg Second-epoch detections are separated by 2.1" and 4.0 pix
The object was found in VSX 4" ZTF J212756.55+352714.4
Type: EW
# Max. Min./Amp. JD0 Period
14.544 r Y 0.276 r 2458423.63010 0.567047200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:56.81 +35:27:16.8: 12.57 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:56.81 +35:27:16.8: 14.06 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212756.55+352714.4,2461185.8480,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212756.55+352714.4 20260525.3480 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.87 21:39:40.95 +34:24:59.2
83.88333 -13.54045 galactic Cyg Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:40.95 +34:24:59.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:40.95 +34:24:59.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:40.95 +34:24:59.2: 14.50 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 21:27:07.34 +35:14:58.4
82.57154 -11.15414 galactic Cyg Second-epoch detections are separated by 7.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:07.34 +35:14:58.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:07.34 +35:14:58.4: 12.47 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:07.34 +35:14:58.4: 14.22 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.82 21:38:09.32 +36:54:28.0
85.38274 -11.50069 galactic Cyg Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951924411105727616 | 21:38:12.46 +36:54:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.567+/- (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:09.32 +36:54:28.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:09.32 +36:54:28.0: 14.05 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951924411105727616,2461185.8480,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951924411105727616 20260525.3480 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.89 21:49:15.19 +35:18:21.5
86.00048 -14.18890 galactic Cyg Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:15.19 +35:18:21.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:15.19 +35:18:21.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:15.19 +35:18:21.5: 14.44 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 22:00:15.80 +35:08:28.9
87.67589 -15.75842 galactic Peg Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948471600995495424 | 22:00:17.55 +35:08:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 1986AJ.....91..144S StKM 1-1958
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:15.80 +35:08:28.9: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:15.80 +35:08:28.9: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948471600995495424,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948471600995495424 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.99 21:32:14.37 +37:49:10.6
85.14544 -10.03143 galactic Cyg Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952247976763269632 | 21:32:14.44 +37:49:44.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.876+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:14.37 +37:49:10.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:14.37 +37:49:10.6: 14.23 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952247976763269632,2461185.8480,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952247976763269632 20260525.3480 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.89 22:02:05.91 +41:42:42.0
92.14541 -10.81972 galactic Lac Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.5172+41.7159 | 22:02:05.91 +41:42:42.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.364+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:05.91 +41:42:42.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:05.91 +41:42:42.0: 14.19 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.5172+41.7159,2461185.8480,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.5172+41.7159 20260525.3480 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.04 21:57:10.60 +42:10:41.6
91.70520 -9.88820 galactic Cyg Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:10.60 +42:10:41.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:10.60 +42:10:41.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:10.60 +42:10:41.6: 14.27 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.89 22:06:23.77 +41:39:59.2
92.76888 -11.34071 galactic Lac Second-epoch detections are separated by 2.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.5987+41.6659 | 22:06:24.91 +41:40:32.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.043 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:23.77 +41:39:59.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:23.77 +41:39:59.2: 13.75 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.5987+41.6659,2461185.8480,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.5987+41.6659 20260525.3480 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.79 21:26:46.13 +37:00:02.7
83.77515 -9.86133 galactic Cyg Second-epoch detections are separated by 6.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1963751960767702144 | 21:26:43.72 +36:59:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:46.13 +37:00:02.7: 13.19 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:46.13 +37:00:02.7: 14.20 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963751960767702144,2461185.8480,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963751960767702144 20260525.3480 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.93 21:56:00.58 +37:10:57.1
88.31982 -13.63348 galactic Cyg Second-epoch detections are separated by 2.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:00.58 +37:10:57.1 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:00.58 +37:10:57.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:00.58 +37:10:57.1: 14.41 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.86 22:04:05.48 +41:13:37.3
92.14722 -11.43146 galactic Lac Second-epoch detections are separated by 0.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959775439522849536 | 22:04:08.19 +41:13:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:05.48 +41:13:37.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:05.48 +41:13:37.3: 13.53 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959775439522849536,2461185.8480,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959775439522849536 20260525.3480 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.99 21:57:11.29 +40:23:42.7
90.57505 -11.28287 galactic Cyg Second-epoch detections are separated by 0.8" and 3.5 pix
The object was found in VSX 2" Gaia DR3 1959308868635915520
Type: ROT
# Max. Min./Amp. JD0 Period
14.470 G 14.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:11.29 +40:23:42.7: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:11.29 +40:23:42.7: 14.10 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959308868635915520,2461185.8480,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959308868635915520 20260525.3480 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.97 22:05:58.50 +41:55:51.3
92.86629 -11.08191 galactic Lac Second-epoch detections are separated by 3.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959835534705997184 | 22:05:58.70 +41:56:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.538+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:58.50 +41:55:51.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:58.50 +41:55:51.3: 13.78 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959835534705997184,2461185.8480,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959835534705997184 20260525.3480 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.95 21:50:34.42 +37:11:03.5
87.46744 -12.93771 galactic Cyg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:34.42 +37:11:03.5 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:34.42 +37:11:03.5: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:34.42 +37:11:03.5: 14.53 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.90 21:59:31.05 +42:08:24.3
92.02702 -10.18690 galactic Lac Second-epoch detections are separated by 3.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960024100952179840 | 21:59:27.28 +42:08:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:31.05 +42:08:24.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:31.05 +42:08:24.3: 14.30 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960024100952179840,2461185.8480,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960024100952179840 20260525.3480 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.07 22:10:36.56 +39:03:13.4
91.83612 -13.91788 galactic Lac Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955525930161165696 | 22:10:39.05 +39:03:41.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE J-Ks=0.326+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:36.56 +39:03:13.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:36.56 +39:03:13.4: 14.34 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955525930161165696,2461185.8480,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955525930161165696 20260525.3480 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.97 21:37:13.77 +40:19:25.1
87.59592 -8.86315 galactic Cyg Second-epoch detections are separated by 2.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1966021868162235520 | 21:37:16.80 +40:18:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:13.77 +40:19:25.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:13.77 +40:19:25.1: 14.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966021868162235520,2461185.8480,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966021868162235520 20260525.3480 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 22:06:38.72 +41:43:51.1
92.84619 -11.31691 galactic Lac Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:38.72 +41:43:51.1 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:38.72 +41:43:51.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:38.72 +41:43:51.1: 14.56 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.90 21:39:53.74 +37:58:53.1
86.38170 -10.94221 galactic Cyg Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953496811513244032 | 21:39:53.19 +37:58:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.542+/-0.097 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:53.74 +37:58:53.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:53.74 +37:58:53.1: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953496811513244032,2461185.8480,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953496811513244032 20260525.3480 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.97 21:48:46.74 +35:26:20.4
86.01517 -14.02508 galactic Cyg Second-epoch detections are separated by 1.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:46.74 +35:26:20.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:46.74 +35:26:20.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:46.74 +35:26:20.4: 14.52 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.90 21:46:54.04 +39:15:19.9
88.28515 -10.89560 galactic Cyg Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:54.04 +39:15:19.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:54.04 +39:15:19.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:54.04 +39:15:19.9: 14.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.91 21:56:34.64 +37:00:25.7
88.29547 -13.84089 galactic Cyg Second-epoch detections are separated by 1.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:34.64 +37:00:25.7 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.787+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:34.64 +37:00:25.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:34.64 +37:00:25.7: 14.41 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.99 21:59:09.95 +36:16:48.9
88.23793 -14.73243 galactic Peg Second-epoch detections are separated by 0.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948789939673020416 | 21:59:09.10 +36:16:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:09.95 +36:16:48.9: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:09.95 +36:16:48.9: 13.61 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948789939673020416,2461185.8480,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948789939673020416 20260525.3480 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 21:39:06.45 +37:40:27.9
86.05385 -11.06428 galactic Cyg Second-epoch detections are separated by 2.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:06.45 +37:40:27.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:06.45 +37:40:27.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:06.45 +37:40:27.9: 14.49 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.98 21:59:27.03 +41:38:40.6
91.70629 -10.56915 galactic Lac Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959940538066922240 | 21:59:28.12 +41:38:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.691+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:27.03 +41:38:40.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:27.03 +41:38:40.6: 14.31 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959940538066922240,2461185.8480,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959940538066922240 20260525.3480 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 21:34:22.92 +34:51:23.4
83.37773 -12.47290 galactic Cyg Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950534972006956032 | 21:34:21.76 +34:52:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:22.92 +34:51:23.4: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:22.92 +34:51:23.4: 14.87 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950534972006956032,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950534972006956032 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.04 22:05:37.91 +35:36:47.0
88.87250 -16.06786 galactic Lac Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948564303570049792 | 22:05:34.99 +35:37:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.738+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:37.91 +35:36:47.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:37.91 +35:36:47.0: 14.62 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948564303570049792,2461185.8480,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948564303570049792 20260525.3480 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.96 22:01:12.35 +35:17:06.2
87.92534 -15.76714 galactic Peg Second-epoch detections are separated by 2.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:12.35 +35:17:06.2 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:12.35 +35:17:06.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:12.35 +35:17:06.2: 14.27 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.02 21:47:32.63 +41:45:11.6
90.02970 -9.07852 galactic Cyg Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.8748+41.7603 | 21:47:29.97 +41:45:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:32.63 +41:45:11.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:32.63 +41:45:11.6: 14.43 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.8748+41.7603,2461185.8480,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.8748+41.7603 20260525.3480 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.94 22:06:02.05 +40:00:16.4
91.69257 -12.62839 galactic Lac Second-epoch detections are separated by 3.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.5220+40.0132 | 22:06:03.77 +40:00:43.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:02.05 +40:00:16.4: 13.20 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:02.05 +40:00:16.4: 14.24 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.5220+40.0132,2461185.8480,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.5220+40.0132 20260525.3480 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.13 21:48:47.80 +38:52:57.8
88.32222 -11.41818 galactic Cyg Second-epoch detections are separated by 4.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:47.80 +38:52:57.8 (user input) | T | P | (position from user input) J-Ks=0.919+/-0.036 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:47.80 +38:52:57.8: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:47.80 +38:52:57.8: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.95 21:47:31.33 +37:36:09.6
87.27557 -12.22546 galactic Cyg Second-epoch detections are separated by 7.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952578414364791680 | 21:47:33.82 +37:35:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:31.33 +37:36:09.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:31.33 +37:36:09.6: 14.04 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952578414364791680,2461185.8480,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952578414364791680 20260525.3480 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.91 21:35:24.09 +36:47:16.4
84.88822 -11.21291 galactic Cyg Second-epoch detections are separated by 1.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951911453183188096 | 21:35:26.01 +36:47:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.737+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:24.09 +36:47:16.4: 12.07 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:24.09 +36:47:16.4: 13.75 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951911453183188096,2461185.8480,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951911453183188096 20260525.3480 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.94 21:41:32.72 +36:23:15.4
85.53679 -12.34343 galactic Cyg Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951089675622432896 | 21:41:34.89 +36:23:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5) J-Ks=0.325+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:32.72 +36:23:15.4: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:32.72 +36:23:15.4: 14.30 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951089675622432896,2461185.8480,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951089675622432896 20260525.3480 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 21:50:58.78 +36:44:37.4
87.23767 -13.32580 galactic Cyg Second-epoch detections are separated by 1.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:58.78 +36:44:37.4 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:58.78 +36:44:37.4: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:58.78 +36:44:37.4: 14.42 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.03 22:00:17.81 +40:36:29.5
91.18242 -11.48302 galactic Lac Second-epoch detections are separated by 4.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959323952561924096 | 22:00:13.80 +40:36:32.3 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.325+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:17.81 +40:36:29.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:17.81 +40:36:29.5: 13.75 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959323952561924096,2461185.8480,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959323952561924096 20260525.3480 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.03 21:46:12.49 +39:34:00.4
88.38935 -10.57267 galactic Cyg Second-epoch detections are separated by 0.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.5447+39.5714 | 21:46:11.37 +39:34:24.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.434+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:12.49 +39:34:00.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:12.49 +39:34:00.4: 13.98 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.5447+39.5714,2461185.8480,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.5447+39.5714 20260525.3480 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.22 21:53:41.44 +40:47:14.5
90.30117 -10.56015 galactic Cyg Second-epoch detections are separated by 4.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:41.44 +40:47:14.5 (user input) | T | P | (position from user input) J-Ks=0.109+/-0.057 (A)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:41.44 +40:47:14.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:41.44 +40:47:14.5: 14.75 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 11.97 21:50:08.02 +34:33:28.4
85.63512 -14.87235 galactic Peg Second-epoch detections are separated by 3.3" and 3.4 pix
The object was found in VSX25" Gaia DR3 1948953668125290368
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.830 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:08.02 +34:33:28.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:08.02 +34:33:28.4: 14.16 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948953668125290368,2461185.8480,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948953668125290368 20260525.3480 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 22:06:37.68 +41:44:03.3
92.84561 -11.31226 galactic Lac Second-epoch detections are separated by 3.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959815125018447488 | 22:06:35.48 +41:44:38.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:37.68 +41:44:03.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:37.68 +41:44:03.3: 14.21 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959815125018447488,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959815125018447488 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.02 21:28:43.59 +35:11:02.7
82.76179 -11.43132 galactic Cyg Second-epoch detections are separated by 0.8" and 3.8 pix
The object was found in VSX 3" Gaia DR3 1951299235669161728
Type: ROT
# Max. Min./Amp. JD0 Period
14.400 G 14.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.59 +35:11:02.7: 13.23 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.59 +35:11:02.7: 14.44 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951299235669161728,2461185.8480,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951299235669161728 20260525.3480 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.01 21:27:00.76 +33:45:02.8
81.47288 -12.19782 galactic Cyg Second-epoch detections are separated by 1.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.7555+33.7505 | 21:27:00.76 +33:45:02.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.381+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:00.76 +33:45:02.8: 12.62 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:00.76 +33:45:02.8: 14.55 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.7555+33.7505,2461185.8480,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.7555+33.7505 20260525.3480 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.20 21:28:43.73 +35:42:02.4
83.13186 -11.06374 galactic Cyg Second-epoch detections are separated by 2.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:43.73 +35:42:02.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.73 +35:42:02.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.73 +35:42:02.4: 15.15 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.09 22:06:09.41 +39:56:12.0
91.66987 -12.69673 galactic Lac Second-epoch detections are separated by 1.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956569401055456768 | 22:06:08.01 +39:56:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.517+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:09.41 +39:56:12.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:09.41 +39:56:12.0: 14.35 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956569401055456768,2461185.8480,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956569401055456768 20260525.3480 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.07 21:44:51.80 +36:12:12.5
85.92085 -12.92689 galactic Cyg Second-epoch detections are separated by 2.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.2141+36.2023 | 21:44:51.80 +36:12:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.696+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:51.80 +36:12:12.5: 12.66 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:51.80 +36:12:12.5: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.2141+36.2023,2461185.8480,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2141+36.2023 20260525.3480 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.19 21:54:32.82 +35:25:31.7
86.92891 -14.79804 galactic Peg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:32.82 +35:25:31.7 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:32.82 +35:25:31.7: 13.30 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:32.82 +35:25:31.7: 15.04 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 22:00:56.16 +36:53:36.2
88.92073 -14.47626 galactic Lac Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2309+36.8928 | 22:00:56.16 +36:53:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:56.16 +36:53:36.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:56.16 +36:53:36.2: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2309+36.8928,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2309+36.8928 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.06 21:47:51.58 +40:21:48.5
89.16132 -10.17488 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1954247369938340736 | 21:47:54.59 +40:21:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:51.58 +40:21:48.5: 13.07 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:51.58 +40:21:48.5: 14.25 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954247369938340736,2461185.8480,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954247369938340736 20260525.3480 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.16 21:40:34.69 +33:42:27.1
83.52745 -14.18667 galactic Cyg Second-epoch detections are separated by 2.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:34.69 +33:42:27.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.534+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:34.69 +33:42:27.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:34.69 +33:42:27.1: 14.71 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.08 21:45:18.29 +37:39:34.8
86.97565 -11.89387 galactic Cyg Second-epoch detections are separated by 0.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952759833784056192 | 21:45:16.89 +37:39:00.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:18.29 +37:39:34.8: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:18.29 +37:39:34.8: 14.57 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952759833784056192,2461185.8480,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952759833784056192 20260525.3480 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.00 22:02:17.99 +35:48:05.0
88.44029 -15.50217 galactic Peg Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1948794238938899840 | 22:02:15.91 +35:48:18.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:17.99 +35:48:05.0: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:17.99 +35:48:05.0: 13.89 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1948794238938899840,2461185.8480,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1948794238938899840 20260525.3480 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 22:04:46.29 +42:08:02.1
92.80856 -10.78536 galactic Lac Second-epoch detections are separated by 0.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1918+42.1233 | 22:04:46.29 +42:08:02.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.843+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:46.29 +42:08:02.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:46.29 +42:08:02.1: 14.30 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1918+42.1233,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1918+42.1233 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.04 21:32:06.91 +39:41:52.6
86.43940 -8.65353 galactic Cyg Second-epoch detections are separated by 2.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:06.91 +39:41:52.6 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:06.91 +39:41:52.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:06.91 +39:41:52.6: 14.34 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:36:58.26 +37:51:36.1
85.86545 -10.64179 galactic Cyg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2508+37.8632 | 21:36:58.26 +37:51:36.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.640+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:58.26 +37:51:36.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:58.26 +37:51:36.1: 14.52 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2508+37.8632,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2508+37.8632 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.09 22:02:38.99 +37:13:44.3
89.41261 -14.42486 galactic Lac Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:38.99 +37:13:44.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:38.99 +37:13:44.3: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:38.99 +37:13:44.3: 14.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.19 21:41:05.04 +34:50:47.1
84.40096 -13.41958 galactic Cyg Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950661140965705344 | 21:41:05.70 +34:51:24.0 (Gaia DR3) | ROT (local) | K (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.458+/-0.060 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:05.04 +34:50:47.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:05.04 +34:50:47.1: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950661140965705344,2461185.8480,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950661140965705344 20260525.3480 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.16 21:29:38.98 +36:14:25.4
83.65219 -10.80877 galactic Cyg Second-epoch detections are separated by 1.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:38.98 +36:14:25.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:38.98 +36:14:25.4: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:38.98 +36:14:25.4: 14.77 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:55:36.33 +35:51:32.4
87.38664 -14.60268 galactic Peg Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949126222734750080 | 21:55:33.00 +35:51:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:36.33 +35:51:32.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:36.33 +35:51:32.4: 14.57 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949126222734750080,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949126222734750080 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.09 21:54:51.04 +40:07:59.2
90.05350 -11.20635 galactic Cyg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was found in VSX20" Gaia DR3 1959389614021445376
Type: ROT
# Max. Min./Amp. JD0 Period
15.060 G 15.100 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:51.04 +40:07:59.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:51.04 +40:07:59.2: 14.46 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959389614021445376,2461185.8480,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959389614021445376 20260525.3480 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 22:01:06.63 +42:14:36.5
92.32816 -10.28656 galactic Lac Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:06.63 +42:14:36.5 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:06.63 +42:14:36.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:06.63 +42:14:36.5: 15.05 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.07 21:49:28.23 +38:12:27.0
87.97693 -12.01733 galactic Cyg Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.3641+38.2092 | 21:49:27.26 +38:11:52.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:28.23 +38:12:27.0: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:28.23 +38:12:27.0: 14.22 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.3641+38.2092,2461185.8480,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.3641+38.2092 20260525.3480 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 22:04:39.48 +41:55:44.1
92.66565 -10.93626 galactic Lac Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1605+41.9291 | 22:04:39.48 +41:55:44.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.448+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:39.48 +41:55:44.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:39.48 +41:55:44.1: 14.76 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1605+41.9291,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1605+41.9291 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 21:50:44.44 +36:27:35.4
87.01083 -13.51076 galactic Peg Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949413745022587008 | 21:50:47.19 +36:27:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.606+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:44.44 +36:27:35.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:44.44 +36:27:35.4: 14.22 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949413745022587008,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949413745022587008 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.22 21:59:42.10 +41:00:46.6
91.34686 -11.09508 galactic Lac Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.9159+41.0218 | 21:59:39.84 +41:01:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:42.10 +41:00:46.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:42.10 +41:00:46.6: 14.68 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9159+41.0218,2461185.8480,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9159+41.0218 20260525.3480 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.25 21:36:16.89 +35:02:27.0
83.79696 -12.60714 galactic Cyg Second-epoch detections are separated by 1.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:16.89 +35:02:27.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:16.89 +35:02:27.0: 13.06 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:16.89 +35:02:27.0: 14.61 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.25 22:08:10.70 +39:02:02.5
91.43352 -13.65273 galactic Lac Second-epoch detections are separated by 0.2" and 3.5 pix
The object was found in VSX 4" Gaia DR3 1956261950116724096
Type: ROT
# Max. Min./Amp. JD0 Period
14.220 G 14.260 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:10.70 +39:02:02.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:10.70 +39:02:02.5: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956261950116724096,2461185.8480,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956261950116724096 20260525.3480 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 21:31:29.68 +33:55:39.8
82.27755 -12.72710 galactic Cyg Second-epoch detections are separated by 1.0" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:29.68 +33:55:39.8 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:29.68 +33:55:39.8: 13.03 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:29.68 +33:55:39.8: 14.42 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 22:04:12.58 +40:40:22.1
91.82246 -11.88588 galactic Lac Second-epoch detections are separated by 2.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956662859543872384 | 22:04:10.82 +40:40:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.625+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:12.58 +40:40:22.1: 12.39 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:12.58 +40:40:22.1: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956662859543872384,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956662859543872384 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.20 21:33:29.30 +37:59:54.7
85.45196 -10.07139 galactic Cyg Second-epoch detections are separated by 0.3" and 3.7 pix
The object was found in VSX17" Gaia DR3 1952276632785584512
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.930 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:29.30 +37:59:54.7: 12.98 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:29.30 +37:59:54.7: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952276632785584512,2461185.8480,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952276632785584512 20260525.3480 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 22:06:29.11 +39:32:46.8
91.48041 -13.04634 galactic Lac Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956338228735784064 | 22:06:32.74 +39:32:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.667+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:29.11 +39:32:46.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:29.11 +39:32:46.8: 14.66 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956338228735784064,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956338228735784064 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 22:00:45.71 +42:12:57.5
92.25919 -10.26876 galactic Lac Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.1869+42.2151 | 22:00:45.71 +42:12:57.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:45.71 +42:12:57.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:45.71 +42:12:57.5: 14.43 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1869+42.2151,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1869+42.2151 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 22:04:43.21 +42:01:06.8
92.73006 -10.87170 galactic Lac Second-epoch detections are separated by 1.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1910+42.0230 | 22:04:43.21 +42:01:06.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.532+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:43.21 +42:01:06.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:43.21 +42:01:06.8: 14.55 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1910+42.0230,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1910+42.0230 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 22:08:49.92 +40:21:08.2
92.34464 -12.66961 galactic Lac Second-epoch detections are separated by 4.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2083+40.3437 | 22:08:49.92 +40:21:08.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:49.92 +40:21:08.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:49.92 +40:21:08.2: 15.21 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2083+40.3437,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2083+40.3437 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.20 21:32:35.91 +35:36:09.9
83.63688 -11.68213 galactic Cyg Second-epoch detections are separated by 1.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.1465+35.6027 | 21:32:35.91 +35:36:09.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:35.91 +35:36:09.9: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:35.91 +35:36:09.9: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.1465+35.6027,2461185.8480,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.1465+35.6027 20260525.3480 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 22:03:59.79 +41:38:51.3
92.39241 -11.08598 galactic Lac Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:59.79 +41:38:51.3 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.058 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:59.79 +41:38:51.3: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:59.79 +41:38:51.3: 14.96 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 22:10:43.52 +41:09:26.3
93.12801 -12.23202 galactic Lac Second-epoch detections are separated by 0.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:43.52 +41:09:26.3 (user input) | T | P | (position from user input) J-Ks=1.088+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:43.52 +41:09:26.3: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:43.52 +41:09:26.3: 14.84 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.09 21:52:14.12 +37:49:46.3
88.15263 -12.65758 galactic Cyg Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952915964435370368 | 21:52:16.76 +37:49:57.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:14.12 +37:49:46.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:14.12 +37:49:46.3: 14.05 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952915964435370368,2461185.8480,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952915964435370368 20260525.3480 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:53:37.65 +42:15:49.5
91.24050 -9.40946 galactic Cyg Second-epoch detections are separated by 0.3" and 3.4 pix
The object was found in VSX 4" Gaia DR3 1960459675052809344
Type: S
# Max. Min./Amp. JD0 Period
15.550 G 16.590 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:37.65 +42:15:49.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:37.65 +42:15:49.5: 14.59 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960459675052809344,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960459675052809344 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.16 22:06:12.37 +39:36:03.7
91.47019 -12.97030 galactic Lac Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:12.37 +39:36:03.7 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:12.37 +39:36:03.7: 13.29 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:12.37 +39:36:03.7: 14.75 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.19 22:04:30.32 +41:26:44.7
92.34529 -11.30430 galactic Lac Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:30.32 +41:26:44.7 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:30.32 +41:26:44.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:30.32 +41:26:44.7: 14.91 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.18 21:58:23.87 +37:48:10.5
89.10044 -13.45094 galactic Lac Second-epoch detections are separated by 2.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:23.87 +37:48:10.5 (user input) | T | P | (position from user input) J-Ks=0.566+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:23.87 +37:48:10.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:23.87 +37:48:10.5: 14.46 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 22:00:09.65 +33:45:56.1
86.75572 -16.81346 galactic Peg Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:09.65 +33:45:56.1 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:09.65 +33:45:56.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:09.65 +33:45:56.1: 14.95 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:35:34.13 +34:35:52.2
83.37591 -12.82839 galactic Cyg Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:34.13 +34:35:52.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:34.13 +34:35:52.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:34.13 +34:35:52.2: 14.70 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 21:30:30.66 +33:57:26.0
82.14936 -12.56326 galactic Cyg Second-epoch detections are separated by 1.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:30.66 +33:57:26.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:30.66 +33:57:26.0: 12.96 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:30.66 +33:57:26.0: 14.54 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.28 21:33:29.11 +33:39:19.5
82.38716 -13.21060 galactic Cyg Second-epoch detections are separated by 3.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:29.11 +33:39:19.5 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:29.11 +33:39:19.5: 12.87 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:29.11 +33:39:19.5: 14.66 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.28 21:52:15.43 +41:18:16.1
90.42290 -9.98909 galactic Cyg Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:15.43 +41:18:16.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:15.43 +41:18:16.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:15.43 +41:18:16.1: 14.65 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:50:17.59 +42:04:56.5
90.64061 -9.15636 galactic Cyg Second-epoch detections are separated by 1.8" and 3.1 pix
The object was found in VSX19" Gaia DR3 1960632160939763456
Type: RS
# Max. Min./Amp. JD0 Period
18.120 G 18.340 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:17.59 +42:04:56.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:17.59 +42:04:56.5: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960632160939763456,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960632160939763456 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 21:52:31.29 +41:07:39.3
90.34748 -10.15716 galactic Cyg Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960243895899781888 | 21:52:28.87 +41:08:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.408+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:31.29 +41:07:39.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:31.29 +41:07:39.3: 14.82 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960243895899781888,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960243895899781888 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:56:04.82 +37:14:36.4
88.37077 -13.59532 galactic Cyg Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:04.82 +37:14:36.4 (user input) | T | P | (position from user input) J-Ks=0.307+/-0.045 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:04.82 +37:14:36.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:04.82 +37:14:36.4: 15.26 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 21:49:25.96 +38:25:18.2
88.11321 -11.84949 galactic Cyg Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:25.96 +38:25:18.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.601+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:25.96 +38:25:18.2: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:25.96 +38:25:18.2: 14.78 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:39:26.02 +34:58:46.9
84.23797 -13.09238 galactic Cyg Second-epoch detections are separated by 2.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:26.02 +34:58:46.9 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.047 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:26.02 +34:58:46.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:26.02 +34:58:46.9: 14.85 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 21:58:33.10 +38:59:49.3
89.89141 -12.53835 galactic Lac Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:33.10 +38:59:49.3 (user input) | T | P | (position from user input) J-Ks=0.230+/-0.037 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:33.10 +38:59:49.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:33.10 +38:59:49.3: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.01 21:26:55.25 +38:03:55.3
84.55541 -9.12508 galactic Cyg Second-epoch detections are separated by 1.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1964230213966061824 | 21:26:54.89 +38:03:17.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.835+/-0.029 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:55.25 +38:03:55.3: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:55.25 +38:03:55.3: 14.52 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1964230213966061824,2461185.8480,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1964230213966061824 20260525.3480 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 22:11:45.13 +41:45:55.6
93.65158 -11.85169 galactic Lac Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:45.13 +41:45:55.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:45.13 +41:45:55.6: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:45.13 +41:45:55.6: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 22:08:58.89 +42:02:06.8
93.38731 -11.33058 galactic Lac Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:58.89 +42:02:06.8 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:58.89 +42:02:06.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:58.89 +42:02:06.8: 15.27 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 22:07:35.18 +41:27:44.3
92.82670 -11.63739 galactic Lac Second-epoch detections are separated by 1.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:35.18 +41:27:44.3 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:35.18 +41:27:44.3: 13.57 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:35.18 +41:27:44.3: 14.44 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 22:05:27.15 +41:32:30.4
92.54865 -11.33459 galactic Lac Second-epoch detections are separated by 0.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:27.15 +41:32:30.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:27.15 +41:32:30.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:27.15 +41:32:30.4: 15.13 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.14 21:56:45.81 +40:47:17.0
90.76144 -10.92596 galactic Cyg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1810+40.7921 | 21:56:45.81 +40:47:17.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.059 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:45.81 +40:47:17.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:45.81 +40:47:17.0: 14.96 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1810+40.7921,2461185.8480,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1810+40.7921 20260525.3480 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.15 21:27:12.50 +33:51:25.4
81.57925 -12.15160 galactic Cyg Second-epoch detections are separated by 3.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.8101+33.8613 | 21:27:12.50 +33:51:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.432+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:12.50 +33:51:25.4: 12.80 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:12.50 +33:51:25.4: 14.22 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.8101+33.8613,2461185.8480,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8101+33.8613 20260525.3480 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.17 21:35:21.65 +41:16:19.3
87.98151 -7.92560 galactic Cyg Second-epoch detections are separated by 4.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.8437+41.2602 | 21:35:21.65 +41:16:19.3 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.387+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:21.65 +41:16:19.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:21.65 +41:16:19.3: 14.60 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8437+41.2602,2461185.8480,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8437+41.2602 20260525.3480 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.17 22:01:09.64 +39:37:09.0
90.69202 -12.36350 galactic Lac Second-epoch detections are separated by 0.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2875+39.6244 | 22:01:09.64 +39:37:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.443+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:09.64 +39:37:09.0: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:09.64 +39:37:09.0: 14.59 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2875+39.6244,2461185.8480,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.2875+39.6244 20260525.3480 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.20 21:40:12.93 +34:16:54.1
83.87224 -13.71407 galactic Cyg Second-epoch detections are separated by 2.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:12.93 +34:16:54.1 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:12.93 +34:16:54.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:12.93 +34:16:54.1: 14.80 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.22 21:34:45.74 +38:35:14.3
86.04643 -9.81392 galactic Cyg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953806568855732608 | 21:34:43.10 +38:35:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.459+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:45.74 +38:35:14.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:45.74 +38:35:14.3: 14.22 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953806568855732608,2461185.8480,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953806568855732608 20260525.3480 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 22:03:08.35 +41:49:49.0
92.37566 -10.84373 galactic Lac Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.7848+41.8332 | 22:03:08.35 +41:49:49.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:08.35 +41:49:49.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:08.35 +41:49:49.0: 15.27 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.7848+41.8332,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.7848+41.8332 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:40:44.27 +35:27:41.7
84.77401 -12.91809 galactic Cyg Second-epoch detections are separated by 1.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:44.27 +35:27:41.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.651+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:44.27 +35:27:41.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:44.27 +35:27:41.7: 15.12 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 22:10:20.81 +41:33:09.1
93.30676 -11.87051 galactic Lac Second-epoch detections are separated by 0.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:10:20.81 +41:33:09.1 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:20.81 +41:33:09.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:20.81 +41:33:09.1: 14.82 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.20 21:36:24.02 +37:34:32.2
85.58435 -10.77346 galactic Cyg Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:24.02 +37:34:32.2 (user input) | T | P | (position from user input) J-Ks=0.762+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:24.02 +37:34:32.2: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:24.02 +37:34:32.2: 14.42 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:43:05.91 +37:32:44.3
86.56418 -11.68958 galactic Cyg Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:05.91 +37:32:44.3 (user input) | T | P | (position from user input) J-Ks=0.764+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:05.91 +37:32:44.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:05.91 +37:32:44.3: 14.80 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.35 21:52:59.24 +34:14:49.0
85.88774 -15.49181 galactic Peg Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:59.24 +34:14:49.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:59.24 +34:14:49.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:59.24 +34:14:49.0: 14.78 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:41:44.91 +34:02:40.1
83.94712 -14.10337 galactic Cyg Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:44.91 +34:02:40.1 (user input) | T | P | (position from user input) J-Ks=0.664+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:44.91 +34:02:40.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:44.91 +34:02:40.1: 14.95 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 22:07:10.96 +38:37:34.4
91.02180 -13.86242 galactic Lac Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:10.96 +38:37:34.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:10.96 +38:37:34.4: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:10.96 +38:37:34.4: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 22:05:48.96 +40:22:58.1
91.89192 -12.30140 galactic Lac Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.4553+40.3936 | 22:05:48.96 +40:22:58.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.636+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:48.96 +40:22:58.1: 13.21 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:48.96 +40:22:58.1: 15.12 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.4553+40.3936,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.4553+40.3936 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 22:10:14.91 +41:02:14.0
92.98138 -12.27628 galactic Lac Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.5647+41.0384 | 22:10:14.91 +41:02:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:14.91 +41:02:14.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:14.91 +41:02:14.0: 15.08 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.5647+41.0384,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.5647+41.0384 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 22:09:51.75 +41:55:24.7
93.45501 -11.51734 galactic Lac Second-epoch detections are separated by 2.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:09:51.75 +41:55:24.7 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:51.75 +41:55:24.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:51.75 +41:55:24.7: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:51:40.11 +38:49:49.1
88.72343 -11.81929 galactic Cyg Second-epoch detections are separated by 0.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:40.11 +38:49:49.1 (user input) | T | P | (position from user input) J-Ks=0.772+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:40.11 +38:49:49.1: 13.12 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:40.11 +38:49:49.1: 14.60 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 22:00:13.75 +41:45:18.1
91.89195 -10.57177 galactic Lac Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.0694+41.7483 | 22:00:16.66 +41:44:54.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.695+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:13.75 +41:45:18.1: 13.34 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:13.75 +41:45:18.1: 15.15 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.0694+41.7483,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.0694+41.7483 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 22:07:23.06 +41:08:43.2
92.60255 -11.86924 galactic Lac Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:23.06 +41:08:43.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:23.06 +41:08:43.2: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:23.06 +41:08:43.2: 15.26 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 21:57:53.26 +36:58:24.0
88.48243 -14.03240 galactic Lac Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:53.26 +36:58:24.0 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.158+/-0.059 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:53.26 +36:58:24.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:53.26 +36:58:24.0: 15.18 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.42 22:00:13.35 +34:58:25.7
87.55968 -15.88350 galactic Peg Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:13.35 +34:58:25.7 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:13.35 +34:58:25.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:13.35 +34:58:25.7: 15.10 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 22:08:34.63 +37:33:22.7
90.58383 -14.88223 galactic Lac Second-epoch detections are separated by 1.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:34.63 +37:33:22.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:34.63 +37:33:22.7: 13.42 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:34.63 +37:33:22.7: 15.40 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.25 22:00:06.38 +39:09:22.8
90.23497 -12.60137 galactic Lac Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.0206+39.1661 | 22:00:06.98 +39:10:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5) J-Ks=0.470+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:06.38 +39:09:22.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:06.38 +39:09:22.8: 14.20 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.0206+39.1661,2461185.8480,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.0206+39.1661 20260525.3480 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:37:32.90 +34:45:17.1
83.79010 -12.99350 galactic Cyg Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:32.90 +34:45:17.1 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:32.90 +34:45:17.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:32.90 +34:45:17.1: 15.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:28:20.93 +36:09:00.3
83.39710 -10.68951 galactic Cyg Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0938+36.1463 | 21:28:20.93 +36:09:00.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:20.93 +36:09:00.3: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:20.93 +36:09:00.3: 14.88 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0938+36.1463,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0938+36.1463 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.28 21:53:14.97 +36:41:36.6
87.56170 -13.65768 galactic Cyg Second-epoch detections are separated by 3.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.3156+36.6914 | 21:53:15.90 +36:42:09.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.381+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:14.97 +36:41:36.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:14.97 +36:41:36.6: 14.59 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.3156+36.6914,2461185.8480,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.3156+36.6914 20260525.3480 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:53:00.65 +35:46:13.8
86.91136 -14.33299 galactic Peg Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:00.65 +35:46:13.8 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.571+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:00.65 +35:46:13.8: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:00.65 +35:46:13.8: 14.74 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:30:41.28 +35:07:19.3
83.00957 -11.75642 galactic Cyg Second-epoch detections are separated by 1.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:41.28 +35:07:19.3 (user input) | T | P | (position from user input) J-Ks=0.710+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:41.28 +35:07:19.3: 13.30 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:41.28 +35:07:19.3: 15.22 +/- 0.32 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.33 22:01:24.44 +41:55:51.4
92.17801 -10.56745 galactic Lac Second-epoch detections are separated by 1.7" and 3.1 pix
The object was found in VSX22" ZTF J220124.12+415529.6
Type: EW
# Max. Min./Amp. JD0 Period
18.566 r Y 0.676 r 2458326.91390 0.258391400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:24.44 +41:55:51.4: 12.85 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:24.44 +41:55:51.4: 14.73 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J220124.12+415529.6,2461185.8480,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J220124.12+415529.6 20260525.3480 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.12 21:30:30.84 +40:52:58.5
87.04057 -7.58433 galactic Cyg Second-epoch detections are separated by 3.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1966991706138848256 | 21:30:28.40 +40:53:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:30.84 +40:52:58.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:30.84 +40:52:58.5: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966991706138848256,2461185.8480,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966991706138848256 20260525.3480 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 21:44:43.69 +35:06:39.2
85.15288 -13.72441 galactic Cyg Second-epoch detections are separated by 0.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1842+35.1101 | 21:44:43.69 +35:06:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.442+/-0.061 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:43.69 +35:06:39.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:43.69 +35:06:39.2: 15.42 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1842+35.1101,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1842+35.1101 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 22:11:07.15 +41:20:25.4
93.29924 -12.12722 galactic Lac Second-epoch detections are separated by 0.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:07.15 +41:20:25.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:07.15 +41:20:25.4: 12.79 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:07.15 +41:20:25.4: 15.24 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:57:39.47 +41:25:20.3
91.29834 -10.53559 galactic Lac Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:39.47 +41:25:20.3 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:39.47 +41:25:20.3: 12.78 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.47 +41:25:20.3: 14.81 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:37:29.63 +35:54:14.5
84.58569 -12.14615 galactic Cyg Second-epoch detections are separated by 2.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.3784+35.8950 | 21:37:29.63 +35:54:14.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.382+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:29.63 +35:54:14.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:29.63 +35:54:14.5: 14.95 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.3784+35.8950,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.3784+35.8950 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:50:22.68 +40:29:52.1
89.62130 -10.38193 galactic Cyg Second-epoch detections are separated by 2.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:22.68 +40:29:52.1 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:22.68 +40:29:52.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:22.68 +40:29:52.1: 15.21 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.53 22:12:24.03 +40:35:38.7
93.05300 -12.87400 galactic Lac Second-epoch detections are separated by 0.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:12:24.03 +40:35:38.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:24.03 +40:35:38.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:24.03 +40:35:38.7: 99.00 +/- 99.00 bad_region
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:35:41.21 +35:13:20.9
83.83415 -12.39160 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was found in VSX 3" Gaia DR3 1950921862659499392
Type: SR|M
# Max. Min./Amp. JD0 Period
13.920 G 14.210 G 45.730000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:41.21 +35:13:20.9: 13.52 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:41.21 +35:13:20.9: 14.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950921862659499392,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950921862659499392 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:36:41.98 +36:15:49.7
84.71668 -11.77364 galactic Cyg Second-epoch detections are separated by 1.2" and 3.8 pix
The object was found in VSX 4" Gaia DR3 1951038788851209984
Type: ROT
# Max. Min./Amp. JD0 Period
15.310 G 15.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:41.98 +36:15:49.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:41.98 +36:15:49.7: 14.75 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951038788851209984,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951038788851209984 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:36:58.91 +34:31:59.2
83.54717 -13.07527 galactic Cyg Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:58.91 +34:31:59.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.436+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:58.91 +34:31:59.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:58.91 +34:31:59.2: 14.74 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:39:50.75 +37:38:28.6
86.14111 -11.18724 galactic Cyg Second-epoch detections are separated by 0.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.9569+37.6477 | 21:39:53.20 +37:38:46.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.469+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:50.75 +37:38:28.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:50.75 +37:38:28.6: 14.90 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.9569+37.6477,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.9569+37.6477 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:30:39.34 +38:36:14.0
85.46759 -9.24976 galactic Cyg Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.6569+38.5994 | 21:30:39.34 +38:36:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.349+/-0.046 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:39.34 +38:36:14.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:39.34 +38:36:14.0: 14.69 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.6569+38.5994,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.6569+38.5994 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 22:03:04.95 +35:09:33.5
88.15557 -16.10434 galactic Peg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:04.95 +35:09:33.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:04.95 +35:09:33.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:04.95 +35:09:33.5: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.28 21:31:32.90 +33:56:49.8
82.29964 -12.72097 galactic Cyg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950356782404057856 | 21:31:35.99 +33:57:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.481+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:32.90 +33:56:49.8: 13.31 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:32.90 +33:56:49.8: 14.67 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950356782404057856,2461185.8480,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950356782404057856 20260525.3480 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 22:07:22.71 +40:35:19.9
92.26172 -12.31488 galactic Lac Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:22.71 +40:35:19.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:22.71 +40:35:19.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:22.71 +40:35:19.9: 14.95 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 22:04:34.65 +36:25:09.6
89.21145 -15.30037 galactic Peg Second-epoch detections are separated by 2.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:34.65 +36:25:09.6 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:34.65 +36:25:09.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:34.65 +36:25:09.6: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:44:23.69 +38:52:48.1
87.66054 -10.85929 galactic Cyg Second-epoch detections are separated by 5.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:23.69 +38:52:48.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:23.69 +38:52:48.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:23.69 +38:52:48.1: 14.69 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:51:39.19 +36:55:28.8
87.46355 -13.27503 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.8989+36.9256 | 21:51:39.19 +36:55:28.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.499+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.19 +36:55:28.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.19 +36:55:28.8: 15.46 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.46 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.8989+36.9256,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.8989+36.9256 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 22:02:22.69 +41:34:47.5
92.10570 -10.95603 galactic Lac Second-epoch detections are separated by 1.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:22.69 +41:34:47.5 (user input) | T | P | (position from user input) J-Ks=0.752+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:22.69 +41:34:47.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:22.69 +41:34:47.5: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:52:45.65 +42:15:35.3
91.11214 -9.31103 galactic Cyg Second-epoch detections are separated by 2.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:45.65 +42:15:35.3 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:45.65 +42:15:35.3: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:45.65 +42:15:35.3: 14.76 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:31:39.39 +36:46:29.2
84.32551 -10.70569 galactic Cyg Second-epoch detections are separated by 2.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:39.39 +36:46:29.2 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:39.39 +36:46:29.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:39.39 +36:46:29.2: 14.42 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:37:58.77 +36:42:07.1
85.21378 -11.62795 galactic Cyg Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951148426473260544 | 21:37:56.76 +36:42:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.544+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:58.77 +36:42:07.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:58.77 +36:42:07.1: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951148426473260544,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951148426473260544 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 22:09:55.37 +40:48:12.0
92.78932 -12.42888 galactic Lac Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.4870+40.8012 | 22:09:55.37 +40:48:12.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:55.37 +40:48:12.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:55.37 +40:48:12.0: 15.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.4870+40.8012,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.4870+40.8012 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:52:44.60 +34:42:49.6
86.16185 -15.10380 galactic Peg Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:44.60 +34:42:49.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:44.60 +34:42:49.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:44.60 +34:42:49.6: 15.36 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 22:05:09.75 +37:59:07.1
90.29677 -14.13247 galactic Lac Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1955080176977684480 | 22:05:09.75 +37:59:07.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:09.75 +37:59:07.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:09.75 +37:59:07.1: 15.15 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1955080176977684480,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1955080176977684480 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.42 21:45:12.02 +40:36:35.5
88.93547 -9.65827 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:12.02 +40:36:35.5 (user input) | T | P | (position from user input) J-Ks=0.787+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:12.02 +40:36:35.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:12.02 +40:36:35.5: 14.95 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:56:15.10 +41:22:11.4
91.05554 -10.41192 galactic Cyg Second-epoch detections are separated by 2.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:56:15.10 +41:22:11.4 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:15.10 +41:22:11.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:15.10 +41:22:11.4: 15.17 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:53:39.07 +34:51:16.0
86.40334 -15.11709 galactic Peg Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.4121+34.8419 | 21:53:39.07 +34:51:16.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:39.07 +34:51:16.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:39.07 +34:51:16.0: 15.20 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.4121+34.8419,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.4121+34.8419 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:50:55.25 +34:16:15.5
85.56790 -15.19556 galactic Peg Second-epoch detections are separated by 3.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948182429438338560 | 21:50:58.21 +34:16:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.472+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:55.25 +34:16:15.5: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:55.25 +34:16:15.5: 14.79 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948182429438338560,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948182429438338560 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:51:03.23 +33:59:27.0
85.39961 -15.42554 galactic Peg Second-epoch detections are separated by 2.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:03.23 +33:59:27.0 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:03.23 +33:59:27.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:03.23 +33:59:27.0: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 22:08:43.68 +41:30:45.0
93.03278 -11.72403 galactic Lac Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:43.68 +41:30:45.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:43.68 +41:30:45.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:43.68 +41:30:45.0: 15.11 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 22:11:12.81 +41:39:57.6
93.50884 -11.87364 galactic Lac Second-epoch detections are separated by 3.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:12.81 +41:39:57.6 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:12.81 +41:39:57.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:12.81 +41:39:57.6: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 22:11:35.58 +41:59:08.7
93.75833 -11.65551 galactic Lac Second-epoch detections are separated by 3.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.8845+41.9884 | 22:11:35.58 +41:59:08.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.665+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:35.58 +41:59:08.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:35.58 +41:59:08.7: 14.68 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.8845+41.9884,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.8845+41.9884 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.28 21:51:22.88 +33:49:09.9
85.33668 -15.59968 galactic Peg Second-epoch detections are separated by 1.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:22.88 +33:49:09.9 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:22.88 +33:49:09.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:22.88 +33:49:09.9: 14.85 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:40:21.22 +39:47:14.7
87.67958 -9.66196 galactic Cyg Second-epoch detections are separated by 1.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:21.22 +39:47:14.7 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.046 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:21.22 +39:47:14.7: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:21.22 +39:47:14.7: 14.87 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 22:11:52.00 +42:03:53.3
93.84755 -11.62093 galactic Lac Second-epoch detections are separated by 4.9" and 2.5 pix
The object was found in VSX23" Gaia DR3 1958289277759126016
Type: ROT
# Max. Min./Amp. JD0 Period
16.250 G 16.290 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:52.00 +42:03:53.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:52.00 +42:03:53.3: 14.81 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958289277759126016,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958289277759126016 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:51:12.70 +35:28:48.9
86.42984 -14.31738 galactic Peg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:12.70 +35:28:48.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:12.70 +35:28:48.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:12.70 +35:28:48.9: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.16 21:27:06.61 +33:44:10.1
81.47690 -12.22251 galactic Cyg Second-epoch detections are separated by 3.0" and 3.5 pix
The object was found in VSX 8" Gaia DR3 1854317224858662912
Type: ROT
# Max. Min./Amp. JD0 Period
15.320 G 15.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:06.61 +33:44:10.1: 12.84 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:06.61 +33:44:10.1: 14.71 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1854317224858662912,2461185.8480,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1854317224858662912 20260525.3480 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 22:05:27.65 +42:00:52.5
92.83954 -10.95764 galactic Lac Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:27.65 +42:00:52.5 (user input) | T | P | (position from user input) J-Ks=1.245+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:27.65 +42:00:52.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:27.65 +42:00:52.5: 15.16 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 22:02:10.53 +42:07:01.9
92.40860 -10.50705 galactic Lac Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1960059250961688832 | 22:02:13.94 +42:07:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:10.53 +42:07:01.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:10.53 +42:07:01.9: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960059250961688832,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960059250961688832 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:29:16.00 +34:53:37.5
82.63408 -11.71569 galactic Cyg Second-epoch detections are separated by 1.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:16.00 +34:53:37.5 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:16.00 +34:53:37.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:16.00 +34:53:37.5: 14.77 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 22:02:41.97 +41:43:44.0
92.24663 -10.87440 galactic Lac Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:41.97 +41:43:44.0 (user input) | T | P | (position from user input) J-Ks=0.621+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:41.97 +41:43:44.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:41.97 +41:43:44.0: 14.95 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 21:53:20.58 +39:06:18.6
89.15866 -11.81637 galactic Cyg Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953146380840621312 | 21:53:19.88 +39:06:49.3 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.473+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:20.58 +39:06:18.6: 12.94 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:20.58 +39:06:18.6: 14.51 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953146380840621312,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953146380840621312 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.19 21:26:51.68 +34:03:09.6
81.66897 -11.96254 galactic Cyg Second-epoch detections are separated by 1.1" and 4.1 pix
The object was found in VSX23" Gaia DR3 1855099733538948736
Type: ROT
# Max. Min./Amp. JD0 Period
16.960 G 17.080 G 0.491688000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:51.68 +34:03:09.6: 13.20 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:51.68 +34:03:09.6: 14.68 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855099733538948736,2461185.8480,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1855099733538948736 20260525.3480 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 21:46:38.91 +34:22:59.8
84.95770 -14.53014 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.6764+34.3835 | 21:46:38.91 +34:22:59.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:38.91 +34:22:59.8: 13.30 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:38.91 +34:22:59.8: 15.28 +/- 0.32 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.6764+34.3835,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.6764+34.3835 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:59:56.19 +38:33:11.5
89.82437 -13.05368 galactic Lac Second-epoch detections are separated by 0.5" and 3.5 pix
The object was found in VSX 3" Gaia DR3 1956022943776768128
Type: E
# Max. Min./Amp. JD0 Period
14.650 G 14.880 G 4.413330000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:56.19 +38:33:11.5: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:56.19 +38:33:11.5: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956022943776768128,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956022943776768128 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.24 21:30:22.42 +38:20:38.9
85.24481 -9.39871 galactic Cyg Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:22.42 +38:20:38.9 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:22.42 +38:20:38.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:22.42 +38:20:38.9: 14.72 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 22:08:02.15 +37:33:32.4
90.49683 -14.81556 galactic Lac Second-epoch detections are separated by 1.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:02.15 +37:33:32.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:02.15 +37:33:32.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:02.15 +37:33:32.4: 15.10 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:33:52.98 +36:12:28.2
84.25564 -11.42470 galactic Cyg Second-epoch detections are separated by 2.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1951777179627181568 | 21:33:55.74 +36:12:41.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.776+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:52.98 +36:12:28.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:52.98 +36:12:28.2: 14.95 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951777179627181568,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951777179627181568 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:40:55.51 +35:54:46.3
85.11487 -12.61055 galactic Cyg Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2405+35.9163 | 21:40:55.51 +35:54:46.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:55.51 +35:54:46.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:55.51 +35:54:46.3: 15.11 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2405+35.9163,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2405+35.9163 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:58:32.72 +37:55:01.1
89.19726 -13.38032 galactic Lac Second-epoch detections are separated by 1.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949965493701517568 | 21:58:29.55 +37:54:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.778+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:32.72 +37:55:01.1: 12.75 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:32.72 +37:55:01.1: 14.63 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949965493701517568,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949965493701517568 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:50:35.57 +37:36:20.8
87.75034 -12.61905 galactic Cyg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:35.57 +37:36:20.8 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:35.57 +37:36:20.8: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:35.57 +37:36:20.8: 14.88 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:29:24.07 +33:58:30.2
81.99434 -12.38901 galactic Cyg Second-epoch detections are separated by 2.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:29:24.07 +33:58:30.2 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:24.07 +33:58:30.2: 12.71 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:24.07 +33:58:30.2: 14.87 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 21:28:04.99 +35:56:21.6
83.20757 -10.80189 galactic Cyg Second-epoch detections are separated by 4.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:04.99 +35:56:21.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:04.99 +35:56:21.6: 12.45 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:04.99 +35:56:21.6: 14.72 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.21 21:31:40.91 +33:48:11.1
82.21675 -12.84342 galactic Cyg Second-epoch detections are separated by 2.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950349841736811008 | 21:31:43.64 +33:47:56.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:40.91 +33:48:11.1: 12.35 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:40.91 +33:48:11.1: 14.59 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950349841736811008,2461185.8480,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950349841736811008 20260525.3480 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:54:19.06 +34:21:38.0
86.18148 -15.58288 galactic Peg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:19.06 +34:21:38.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:19.06 +34:21:38.0: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:19.06 +34:21:38.0: 14.55 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 22:10:15.85 +41:34:00.4
93.30254 -11.84990 galactic Lac Second-epoch detections are separated by 1.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.5657+41.5671 | 22:10:15.85 +41:34:00.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.696+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:15.85 +41:34:00.4: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:15.85 +41:34:00.4: 14.86 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.5657+41.5671,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.5657+41.5671 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:26:53.85 +33:43:13.3
81.43354 -12.20230 galactic Cyg Second-epoch detections are separated by 4.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:26:53.85 +33:43:13.3 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:53.85 +33:43:13.3: 12.62 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:53.85 +33:43:13.3: 14.85 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:33:23.27 +35:48:05.1
83.89539 -11.64967 galactic Cyg Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.3474+35.8101 | 21:33:23.27 +35:48:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.311+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:23.27 +35:48:05.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:23.27 +35:48:05.1: 14.62 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.3474+35.8101,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.3474+35.8101 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.17 21:32:38.78 +34:43:55.9
83.02644 -12.31572 galactic Cyg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:38.78 +34:43:55.9 (user input) | T | P | (position from user input) J-Ks=0.853+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:38.78 +34:43:55.9: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:38.78 +34:43:55.9: 14.29 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:59:50.53 +41:52:08.1
91.90546 -10.43763 galactic Lac Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:50.53 +41:52:08.1 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:50.53 +41:52:08.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:50.53 +41:52:08.1: 14.81 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 21:58:43.93 +39:44:49.6
90.39786 -11.97363 galactic Lac Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6842+39.7459 | 21:58:43.93 +39:44:49.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:43.93 +39:44:49.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:43.93 +39:44:49.6: 14.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6842+39.7459,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6842+39.7459 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:34:30.55 +33:45:42.3
82.62051 -13.28178 galactic Cyg Second-epoch detections are separated by 2.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:30.55 +33:45:42.3 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:30.55 +33:45:42.3: 13.46 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:30.55 +33:45:42.3: 14.90 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:58:36.26 +41:09:23.1
91.27193 -10.85440 galactic Lac Second-epoch detections are separated by 0.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:36.26 +41:09:23.1 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:36.26 +41:09:23.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:36.26 +41:09:23.1: 14.77 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.28 21:50:53.08 +37:38:05.3
87.81474 -12.63430 galactic Cyg Second-epoch detections are separated by 2.4" and 3.5 pix
The object was found in VSX 9" Gaia DR3 1952900463893673728
Type: ROT
# Max. Min./Amp. JD0 Period
17.590 G 17.650 G 0.319524000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:53.08 +37:38:05.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:53.08 +37:38:05.3: 14.59 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952900463893673728,2461185.8480,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952900463893673728 20260525.3480 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:52:19.93 +39:44:46.8
89.42296 -11.19820 galactic Cyg Second-epoch detections are separated by 1.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.0824+39.7460 | 21:52:18.41 +39:45:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:19.93 +39:44:46.8: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:19.93 +39:44:46.8: 14.23 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.0824+39.7460,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.0824+39.7460 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 22:04:44.36 +37:33:00.6
89.95450 -14.42626 galactic Lac Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:44.36 +37:33:00.6 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:44.36 +37:33:00.6: 13.23 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:44.36 +37:33:00.6: 15.26 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 22:07:31.14 +39:46:41.6
91.78662 -12.98043 galactic Lac Second-epoch detections are separated by 5.3" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:07:31.14 +39:46:41.6 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:31.14 +39:46:41.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:31.14 +39:46:41.6: 15.45 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.45 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 22:03:12.98 +39:06:03.2
90.68721 -13.01654 galactic Lac Second-epoch detections are separated by 0.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:12.98 +39:06:03.2 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:12.98 +39:06:03.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:12.98 +39:06:03.2: 14.94 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:31:57.30 +36:19:02.3
84.04650 -11.07691 galactic Cyg Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:57.30 +36:19:02.3 (user input) | T | P | (position from user input) J-Ks=0.708+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:57.30 +36:19:02.3: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:57.30 +36:19:02.3: 14.62 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:51:11.92 +37:00:41.8
87.45014 -13.15000 galactic Cyg Second-epoch detections are separated by 2.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949490156780126336 | 21:51:09.14 +37:01:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.426+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:11.92 +37:00:41.8: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:11.92 +37:00:41.8: 14.63 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949490156780126336,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949490156780126336 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:42:31.31 +35:51:14.4
85.31988 -12.87146 galactic Cyg Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6327+35.8537 | 21:42:31.31 +35:51:14.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:31.31 +35:51:14.4: 13.39 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:31.31 +35:51:14.4: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.6327+35.8537,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6327+35.8537 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:39:23.59 +37:37:07.9
86.05820 -11.14343 galactic Cyg Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953463177628661888 | 21:39:22.97 +37:36:25.9 (Gaia DR3) | E (local) | K (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.378+/-0.063 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:23.59 +37:37:07.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:23.59 +37:37:07.9: 14.68 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953463177628661888,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953463177628661888 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:28:08.29 +36:20:37.2
83.50450 -10.52178 galactic Cyg Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0319+36.3316 | 21:28:08.29 +36:20:37.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:08.29 +36:20:37.2: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:08.29 +36:20:37.2: 14.85 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0319+36.3316,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0319+36.3316 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:37:02.85 +36:17:37.9
84.78998 -11.79951 galactic Cyg Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:02.85 +36:17:37.9 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:02.85 +36:17:37.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:02.85 +36:17:37.9: 14.89 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:29:00.99 +33:49:52.9
81.83274 -12.43493 galactic Cyg Second-epoch detections are separated by 2.2" and 4.1 pix
The object was found in VSX19" ZTF J212859.55+334957.8
Type: BY
# Max. Min./Amp. JD0 Period
16.769 r Y 0.091 r 2458218.97490 0.387821700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:00.99 +33:49:52.9: 12.86 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:00.99 +33:49:52.9: 14.93 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J212859.55+334957.8,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212859.55+334957.8 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:54:45.91 +38:18:19.5
88.85678 -12.60979 galactic Cyg Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:45.91 +38:18:19.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.436+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:45.91 +38:18:19.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:45.91 +38:18:19.5: 14.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:50:56.50 +33:55:09.6
85.33284 -15.46440 galactic Peg Second-epoch detections are separated by 0.6" and 3.8 pix
The object was found in VSX15" Gaia DR3 1946660911504210304
Type: ROT
# Max. Min./Amp. JD0 Period
16.080 G 16.120 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:56.50 +33:55:09.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:56.50 +33:55:09.6: 14.80 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1946660911504210304,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1946660911504210304 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:58:49.54 +40:28:43.1
90.87662 -11.41180 galactic Lac Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:49.54 +40:28:43.1 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:49.54 +40:28:43.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:49.54 +40:28:43.1: 14.98 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 22:08:28.16 +41:17:32.5
92.85952 -11.87252 galactic Lac Second-epoch detections are separated by 0.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:28.16 +41:17:32.5 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:28.16 +41:17:32.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:28.16 +41:17:32.5: 15.29 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 21:55:07.10 +38:37:59.5
89.12458 -12.40037 galactic Cyg Second-epoch detections are separated by 2.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:07.10 +38:37:59.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:07.10 +38:37:59.5: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:07.10 +38:37:59.5: 15.27 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:28:55.84 +39:02:12.2
85.52708 -8.70498 galactic Cyg Second-epoch detections are separated by 3.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:55.84 +39:02:12.2 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:55.84 +39:02:12.2: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:55.84 +39:02:12.2: 15.01 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 21:30:33.16 +34:04:09.8
82.23618 -12.48928 galactic Cyg Second-epoch detections are separated by 1.2" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:33.16 +34:04:09.8 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:33.16 +34:04:09.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:33.16 +34:04:09.8: 14.65 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 21:47:46.25 +35:56:49.8
86.19989 -13.50744 galactic Cyg Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:46.25 +35:56:49.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:46.25 +35:56:49.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:46.25 +35:56:49.8: 14.94 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:43:50.45 +37:03:22.9
86.34422 -12.15312 galactic Cyg Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.9599+37.0575 | 21:43:50.45 +37:03:22.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:50.45 +37:03:22.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:50.45 +37:03:22.9: 14.77 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.9599+37.0575,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.9599+37.0575 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.35 21:50:07.74 +42:10:51.9
90.68101 -9.06106 galactic Cyg Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.5325+42.1739 | 21:50:07.74 +42:10:51.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.441+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:07.74 +42:10:51.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:07.74 +42:10:51.9: 14.61 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.5325+42.1739,2461185.8480,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.5325+42.1739 20260525.3480 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:31:26.89 +33:46:05.5
82.15613 -12.83444 galactic Cyg Second-epoch detections are separated by 0.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:26.89 +33:46:05.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:26.89 +33:46:05.5: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:26.89 +33:46:05.5: 14.53 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:49:09.64 +42:12:56.5
90.56432 -8.91937 galactic Cyg Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:09.64 +42:12:56.5 (user input) | T | P | (position from user input) J-Ks=0.792+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:09.64 +42:12:56.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:09.64 +42:12:56.5: 15.31 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:56:26.04 +37:57:07.1
88.88747 -13.09118 galactic Cyg Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1061+37.9513 | 21:56:26.04 +37:57:07.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.698+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:26.04 +37:57:07.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:26.04 +37:57:07.1: 14.78 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1061+37.9513,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1061+37.9513 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 22:12:02.15 +41:01:53.3
93.25740 -12.47864 galactic Lac Second-epoch detections are separated by 3.8" and 2.7 pix
The object was found in VSX18" Gaia DR3 1958025218872059392
Type: ROT
# Max. Min./Amp. JD0 Period
18.280 G 18.490 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:02.15 +41:01:53.3: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:02.15 +41:01:53.3: 14.94 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958025218872059392,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958025218872059392 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 22:03:19.70 +38:40:39.2
90.43875 -13.36463 galactic Lac Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955908006151463040 | 22:03:18.81 +38:40:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:19.70 +38:40:39.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:19.70 +38:40:39.2: 14.45 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955908006151463040,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955908006151463040 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:47:53.10 +34:00:34.1
84.89965 -14.97953 galactic Cyg Second-epoch detections are separated by 3.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:53.10 +34:00:34.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:53.10 +34:00:34.1: 12.88 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:53.10 +34:00:34.1: 14.99 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:49:59.42 +34:39:56.9
85.68517 -14.77148 galactic Peg Second-epoch detections are separated by 2.4" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:59.42 +34:39:56.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:59.42 +34:39:56.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:59.42 +34:39:56.9: 14.63 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.50 22:08:12.38 +39:44:12.0
91.86979 -13.09274 galactic Lac Second-epoch detections are separated by 4.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:12.38 +39:44:12.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:12.38 +39:44:12.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:12.38 +39:44:12.0: 14.50 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:46:56.92 +41:43:39.2
89.92728 -9.02602 galactic Cyg Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.7346+41.7185 | 21:46:56.92 +41:43:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.885+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:56.92 +41:43:39.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:56.92 +41:43:39.2: 14.66 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.7346+41.7185,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.7346+41.7185 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:36:08.48 +35:55:06.2
84.39124 -11.94856 galactic Cyg Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:08.48 +35:55:06.2 (user input) | T | P | (position from user input) J-Ks=0.537+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:08.48 +35:55:06.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:08.48 +35:55:06.2: 14.36 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 22:06:05.56 +41:38:13.1
92.70457 -11.33034 galactic Lac Second-epoch detections are separated by 2.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:05.56 +41:38:13.1 (user input) | T | P | (position from user input) J-Ks=0.639+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:05.56 +41:38:13.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:05.56 +41:38:13.1: 14.98 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:45:54.78 +36:04:45.0
85.99917 -13.16043 galactic Cyg Second-epoch detections are separated by 2.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.4723+36.0738 | 21:45:54.78 +36:04:45.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.370+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:54.78 +36:04:45.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:54.78 +36:04:45.0: 14.72 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.4723+36.0738,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.4723+36.0738 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:43:24.22 +39:02:44.7
87.62496 -10.60756 galactic Cyg Second-epoch detections are separated by 1.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:24.22 +39:02:44.7 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:24.22 +39:02:44.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:24.22 +39:02:44.7: 14.97 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.26 21:54:13.84 +42:03:14.7
91.19423 -9.64264 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:13.84 +42:03:14.7 (user input) | T | P | (position from user input) J-Ks=0.806+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:13.84 +42:03:14.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:13.84 +42:03:14.7: 14.92 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.49 22:03:45.58 +37:16:45.0
89.62424 -14.52129 galactic Lac Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:45.58 +37:16:45.0 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:45.58 +37:16:45.0: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:45.58 +37:16:45.0: 15.36 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:58:01.47 +38:57:27.0
89.78418 -12.50516 galactic Lac Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:01.47 +38:57:27.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.818+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:01.47 +38:57:27.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:01.47 +38:57:27.0: 15.26 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:49:19.26 +36:58:39.0
87.13471 -12.93252 galactic Cyg Second-epoch detections are separated by 0.8" and 3.7 pix
The object was found in VSX23" Gaia DR3 1952490006758391552
Type: VAR
# Max. Min./Amp. JD0 Period
16.270 G 16.290 G 0.019761600000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:19.26 +36:58:39.0: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:19.26 +36:58:39.0: 14.92 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952490006758391552,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952490006758391552 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:52:57.14 +41:56:24.0
90.93445 -9.58086 galactic Cyg Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:52:57.14 +41:56:24.0 (user input) | T | P | (position from user input) J-Ks=0.547+/-0.098 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:57.14 +41:56:24.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:57.14 +41:56:24.0: 14.78 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:59:54.31 +34:16:50.9
87.05242 -16.38055 galactic Peg Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:54.31 +34:16:50.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:54.31 +34:16:50.9: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:54.31 +34:16:50.9: 15.19 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 21:55:11.88 +36:28:56.0
87.73183 -14.07040 galactic Peg Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:11.88 +36:28:56.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:11.88 +36:28:56.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:11.88 +36:28:56.0: 14.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 22:01:30.08 +41:04:28.8
91.65823 -11.25523 galactic Lac Second-epoch detections are separated by 0.8" and 3.5 pix
The object was found in VSX 2" Gaia DR3 1959712217606533504
Type:
# Max. Min./Amp. JD0 Period
15.750 G 16.070 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:30.08 +41:04:28.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:30.08 +41:04:28.8: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959712217606533504,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959712217606533504 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.35 22:00:40.88 +34:40:45.0
87.44321 -16.17185 galactic Peg Second-epoch detections are separated by 3.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1948440745946028672 | 22:00:41.45 +34:40:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:40.88 +34:40:45.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:40.88 +34:40:45.0: 14.43 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948440745946028672,2461185.8480,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948440745946028672 20260525.3480 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:28:15.82 +34:43:42.3
82.36586 -11.68854 galactic Cyg Second-epoch detections are separated by 2.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0699+34.7159 | 21:28:15.82 +34:43:42.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.332+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:15.82 +34:43:42.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:15.82 +34:43:42.3: 14.49 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0699+34.7159,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0699+34.7159 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:33:16.16 +41:46:48.3
88.04095 -7.28695 galactic Cyg Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.3240+41.7774 | 21:33:16.16 +41:46:48.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.474+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:16.16 +41:46:48.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:16.16 +41:46:48.3: 14.39 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.3240+41.7774,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.3240+41.7774 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 22:00:20.90 +41:35:27.5
91.80712 -10.71480 galactic Lac Second-epoch detections are separated by 1.5" and 3.3 pix
The object was found in VSX 2" Gaia DR3 1959950433671965952
Type: E
# Max. Min./Amp. JD0 Period
14.760 G 14.940 G 15.274000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:20.90 +41:35:27.5: 13.25 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:20.90 +41:35:27.5: 15.24 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959950433671965952,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959950433671965952 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 22:08:56.95 +41:29:27.8
93.05389 -11.76583 galactic Lac Second-epoch detections are separated by 0.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:56.95 +41:29:27.8 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:56.95 +41:29:27.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:56.95 +41:29:27.8: 15.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:58:48.24 +40:45:27.6
91.04997 -11.19049 galactic Lac Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959343125295495168 | 21:58:45.44 +40:45:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.410+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:48.24 +40:45:27.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:48.24 +40:45:27.6: 15.29 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959343125295495168,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959343125295495168 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:38:03.92 +38:03:50.8
86.16757 -10.63803 galactic Cyg Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:03.92 +38:03:50.8 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.042 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:03.92 +38:03:50.8: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:03.92 +38:03:50.8: 14.77 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:48:31.78 +39:16:35.8
88.54284 -11.08499 galactic Cyg Second-epoch detections are separated by 1.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.1228+39.2740 | 21:48:31.78 +39:16:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.531+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:31.78 +39:16:35.8: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:31.78 +39:16:35.8: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.1228+39.2740,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1228+39.2740 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:55:20.84 +34:39:46.5
86.55194 -15.48791 galactic Peg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:20.84 +34:39:46.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:20.84 +34:39:46.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:20.84 +34:39:46.5: 14.92 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:42:21.52 +36:16:15.6
85.58116 -12.53978 galactic Cyg Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5847+36.2720 | 21:42:21.52 +36:16:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.622+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:21.52 +36:16:15.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:21.52 +36:16:15.6: 14.76 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5847+36.2720,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5847+36.2720 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 22:02:43.72 +35:30:17.9
88.31997 -15.78857 galactic Peg Second-epoch detections are separated by 1.9" and 3.7 pix
The object was found in VSX 5" Gaia DR3 1948586706118950016
Type: ROT
# Max. Min./Amp. JD0 Period
15.860 G 15.920 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:43.72 +35:30:17.9: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:43.72 +35:30:17.9: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948586706118950016,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948586706118950016 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.49 21:34:31.83 +40:00:34.5
86.99701 -8.74396 galactic Cyg Second-epoch detections are separated by 2.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.6318+40.0063 | 21:34:31.83 +40:00:34.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.745+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:31.83 +40:00:34.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:31.83 +40:00:34.5: 14.65 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.6318+40.0063,2461185.8480,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.6318+40.0063 20260525.3480 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:54:17.40 +36:52:10.6
87.84243 -13.65605 galactic Cyg Second-epoch detections are separated by 0.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:17.40 +36:52:10.6 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:17.40 +36:52:10.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:17.40 +36:52:10.6: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:37:03.51 +37:31:36.8
85.64791 -10.89793 galactic Cyg Second-epoch detections are separated by 1.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:03.51 +37:31:36.8 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:03.51 +37:31:36.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:03.51 +37:31:36.8: 14.98 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 22:04:39.71 +37:04:27.3
89.64108 -14.79335 galactic Lac Second-epoch detections are separated by 1.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:39.71 +37:04:27.3 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:39.71 +37:04:27.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:39.71 +37:04:27.3: 15.16 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:57:38.67 +36:43:41.1
88.28400 -14.19203 galactic Cyg Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1949565546349700224 | 21:57:40.83 +36:43:11.3 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:38.67 +36:43:41.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:38.67 +36:43:41.1: 14.01 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949565546349700224,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949565546349700224 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:59:07.04 +37:35:41.8
89.08055 -13.70221 galactic Lac Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.7788+37.5953 | 21:59:07.04 +37:35:41.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.319+/-0.057 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:07.04 +37:35:41.8: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:07.04 +37:35:41.8: 15.23 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.7788+37.5953,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.7788+37.5953 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 21:29:05.04 +40:36:55.7
86.65662 -7.59004 galactic Cyg Second-epoch detections are separated by 3.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.2729+40.6150 | 21:29:05.04 +40:36:55.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:05.04 +40:36:55.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:05.04 +40:36:55.7: 14.60 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.2729+40.6150,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.2729+40.6150 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:33:40.02 +33:37:46.0
82.39658 -13.25558 galactic Cyg Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:40.02 +33:37:46.0 (user input) | T | P | (position from user input) J-Ks=0.624+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:40.02 +33:37:46.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:40.02 +33:37:46.0: 14.91 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:33:43.05 +37:03:45.6
84.83110 -10.78206 galactic Cyg Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.4299+37.0630 | 21:33:43.05 +37:03:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.449+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:43.05 +37:03:45.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:43.05 +37:03:45.6: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4299+37.0630,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4299+37.0630 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.58 22:08:55.68 +38:16:52.9
91.09020 -14.34334 galactic Lac Second-epoch detections are separated by 2.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:08:55.68 +38:16:52.9 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:55.68 +38:16:52.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:55.68 +38:16:52.9: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.49 21:53:51.27 +33:51:00.5
85.76274 -15.91043 galactic Peg Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.4615+33.8519 | 21:53:51.27 +33:51:00.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.501+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:51.27 +33:51:00.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:51.27 +33:51:00.5: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.4615+33.8519,2461185.8480,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.4615+33.8519 20260525.3480 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 21:27:30.62 +35:18:41.9
82.67339 -11.16598 galactic Cyg Second-epoch detections are separated by 6.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.8779+35.3116 | 21:27:30.62 +35:18:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.628+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:30.62 +35:18:41.9: 12.56 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:30.62 +35:18:41.9: 14.31 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.8779+35.3116,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8779+35.3116 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.42 21:51:39.59 +40:18:36.0
89.68925 -10.68252 galactic Cyg Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:39.59 +40:18:36.0 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.59 +40:18:36.0: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.59 +40:18:36.0: 14.87 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.49 22:02:49.10 +35:57:04.6
88.62227 -15.44981 galactic Peg Second-epoch detections are separated by 2.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:49.10 +35:57:04.6 (user input) | T | P | (position from user input) J-Ks=0.582+/- (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:49.10 +35:57:04.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:49.10 +35:57:04.6: 15.27 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:37:17.02 +36:54:05.4
85.24793 -11.38692 galactic Cyg Second-epoch detections are separated by 2.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:17.02 +36:54:05.4 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:17.02 +36:54:05.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:17.02 +36:54:05.4: 15.04 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:49:30.28 +38:28:52.1
88.16354 -11.81340 galactic Cyg Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:30.28 +38:28:52.1 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:30.28 +38:28:52.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:30.28 +38:28:52.1: 15.33 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.25 21:28:43.48 +36:04:03.7
83.39337 -10.80148 galactic Cyg Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:43.48 +36:04:03.7 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.48 +36:04:03.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.48 +36:04:03.7: 14.89 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 22:00:10.43 +38:33:13.9
89.86212 -13.08198 galactic Lac Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:10.43 +38:33:13.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.413+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:10.43 +38:33:13.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:10.43 +38:33:13.9: 14.90 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.35 22:11:52.66 +40:52:48.1
93.14190 -12.58408 galactic Lac Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:52.66 +40:52:48.1 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:52.66 +40:52:48.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:52.66 +40:52:48.1: 14.73 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:43:28.90 +37:46:48.1
86.78112 -11.56494 galactic Cyg Second-epoch detections are separated by 1.5" and 3.7 pix
The object was found in VSX19" Gaia DR3 1952809964643278080
Type: RS
# Max. Min./Amp. JD0 Period
16.190 G 16.250 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:28.90 +37:46:48.1: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:28.90 +37:46:48.1: 14.69 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952809964643278080,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952809964643278080 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:34:28.42 +40:12:23.8
87.12486 -8.59243 galactic Cyg Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.6187+40.2067 | 21:34:28.42 +40:12:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.292+/-0.044 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:28.42 +40:12:23.8: 12.74 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:28.42 +40:12:23.8: 15.03 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.6187+40.2067,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.6187+40.2067 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.57 22:11:50.18 +39:03:26.3
92.03646 -14.05558 galactic Lac Second-epoch detections are separated by 2.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:50.18 +39:03:26.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:50.18 +39:03:26.3: 13.44 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:50.18 +39:03:26.3: 15.27 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 22:03:00.73 +38:51:52.9
90.50650 -13.17897 galactic Lac Second-epoch detections are separated by 3.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955930894037355904 | 22:03:03.27 +38:52:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.481+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:00.73 +38:51:52.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:00.73 +38:51:52.9: 15.00 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955930894037355904,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955930894037355904 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:57:52.96 +34:06:45.3
86.60432 -16.24548 galactic Peg Second-epoch detections are separated by 5.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:52.96 +34:06:45.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:52.96 +34:06:45.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:52.96 +34:06:45.3: 15.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:49:13.72 +35:11:21.8
85.91775 -14.27367 galactic Cyg Second-epoch detections are separated by 2.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:13.72 +35:11:21.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:13.72 +35:11:21.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:13.72 +35:11:21.8: 14.96 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.35 22:02:05.34 +37:22:23.9
89.41413 -14.24246 galactic Lac Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:05.34 +37:22:23.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:05.34 +37:22:23.9: 12.65 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:05.34 +37:22:23.9: 15.13 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.42 21:57:21.27 +37:30:14.8
88.74208 -13.55344 galactic Cyg Second-epoch detections are separated by 1.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:57:21.27 +37:30:14.8 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:21.27 +37:30:14.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:21.27 +37:30:14.8: 15.33 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:42:25.14 +35:54:12.6
85.33805 -12.82076 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5931+35.9084 | 21:42:25.14 +35:54:12.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.470+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:25.14 +35:54:12.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:25.14 +35:54:12.6: 14.80 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5931+35.9084,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5931+35.9084 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 21:48:39.22 +37:49:35.3
87.59851 -12.20218 galactic Cyg Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:39.22 +37:49:35.3 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:39.22 +37:49:35.3: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:39.22 +37:49:35.3: 15.23 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:44:01.36 +38:56:13.3
87.64353 -10.76867 galactic Cyg Second-epoch detections are separated by 2.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1954018053043260288 | 21:44:03.28 +38:56:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.609+/-0.041 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:01.36 +38:56:13.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:01.36 +38:56:13.3: 14.62 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954018053043260288,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954018053043260288 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:34:10.50 +35:44:49.6
83.97509 -11.79917 galactic Cyg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.5393+35.7372 | 21:34:10.50 +35:44:49.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.361+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:10.50 +35:44:49.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:10.50 +35:44:49.6: 14.63 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.5393+35.7372,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.5393+35.7372 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.50 22:01:39.44 +34:45:27.5
87.65716 -16.23645 galactic Peg Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.4101+34.7686 | 22:01:39.44 +34:45:27.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.234+/-0.048 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:39.44 +34:45:27.5: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:39.44 +34:45:27.5: 15.34 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.34 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.4101+34.7686,2461185.8480,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.4101+34.7686 20260525.3480 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.31 22:00:37.79 +41:43:04.1
91.92866 -10.64707 galactic Lac Second-epoch detections are separated by 1.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.1728+41.7134 | 22:00:37.79 +41:43:04.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:37.79 +41:43:04.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:37.79 +41:43:04.1: 14.76 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1728+41.7134,2461185.8480,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1728+41.7134 20260525.3480 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:54:53.71 +41:04:43.2
90.66774 -10.47820 galactic Cyg Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:53.71 +41:04:43.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:53.71 +41:04:43.2: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:53.71 +41:04:43.2: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 21:29:44.17 +35:02:48.4
82.81368 -11.67402 galactic Cyg Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1951246871423742464 | 21:29:44.17 +35:02:48.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:44.17 +35:02:48.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:44.17 +35:02:48.4: 15.24 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1951246871423742464,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1951246871423742464 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:59:17.07 +35:39:25.5
87.85151 -15.23200 galactic Peg Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:17.07 +35:39:25.5 (user input) | T | P | (position from user input) J-Ks=0.598+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:17.07 +35:39:25.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:17.07 +35:39:25.5: 15.26 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:41:58.03 +35:21:26.8
84.89198 -13.16382 galactic Cyg Second-epoch detections are separated by 1.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4903+35.3504 | 21:41:58.03 +35:21:26.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:58.03 +35:21:26.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:58.03 +35:21:26.8: 14.78 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4903+35.3504,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4903+35.3504 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 22:04:41.21 +40:20:51.2
91.69472 -12.19958 galactic Lac Second-epoch detections are separated by 1.1" and 3.3 pix
The object was found in VSX15" Gaia DR3 1956639769799538560
Type: ROT
# Max. Min./Amp. JD0 Period
15.840 G 15.880 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:41.21 +40:20:51.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:41.21 +40:20:51.2: 14.51 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956639769799538560,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956639769799538560 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.53 22:00:13.59 +38:25:18.0
89.78611 -13.19199 galactic Lac Second-epoch detections are separated by 0.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:13.59 +38:25:18.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.810+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:13.59 +38:25:18.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:13.59 +38:25:18.0: 15.26 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:46:22.62 +36:17:37.7
86.21696 -13.06123 galactic Cyg Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1952352529144641152 | 21:46:22.12 +36:17:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:22.62 +36:17:37.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:22.62 +36:17:37.7: 14.35 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952352529144641152,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952352529144641152 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:36:08.38 +34:28:55.9
83.38180 -12.99319 galactic Cyg Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:08.38 +34:28:55.9 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.046 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:08.38 +34:28:55.9: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:08.38 +34:28:55.9: 15.01 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:58:26.35 +42:12:16.4
91.90791 -10.01276 galactic Lac Second-epoch detections are separated by 0.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:26.35 +42:12:16.4 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:26.35 +42:12:16.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:26.35 +42:12:16.4: 15.18 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:35:23.86 +34:51:32.9
83.53419 -12.61466 galactic Cyg Second-epoch detections are separated by 1.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:23.86 +34:51:32.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.713+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:23.86 +34:51:32.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:23.86 +34:51:32.9: 15.07 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:31:17.69 +33:40:29.1
82.06571 -12.87892 galactic Cyg Second-epoch detections are separated by 1.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:17.69 +33:40:29.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:17.69 +33:40:29.1: 12.98 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:17.69 +33:40:29.1: 15.15 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.40 22:04:51.38 +36:57:57.2
89.60421 -14.90280 galactic Lac Second-epoch detections are separated by 0.4" and 3.6 pix
The object was found in VSX 1" Gaia DR3 1954873507448471680
Type: RS
# Max. Min./Amp. JD0 Period
15.100 G 15.210 G 0.369502000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:51.38 +36:57:57.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:51.38 +36:57:57.2: 15.11 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954873507448471680,2461185.8480,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954873507448471680 20260525.3480 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 22:06:53.62 +39:49:46.3
91.71959 -12.86735 galactic Lac Second-epoch detections are separated by 1.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:53.62 +39:49:46.3 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:53.62 +39:49:46.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:53.62 +39:49:46.3: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:33:24.09 +35:46:28.4
83.87848 -11.67100 galactic Cyg Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:24.09 +35:46:28.4 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:24.09 +35:46:28.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:24.09 +35:46:28.4: 15.11 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:39:07.59 +35:00:10.2
84.20672 -13.03266 galactic Cyg Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:07.59 +35:00:10.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:07.59 +35:00:10.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:07.59 +35:00:10.2: 15.05 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 22:12:09.67 +41:33:21.3
93.59010 -12.06645 galactic Lac Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:12:09.67 +41:33:21.3 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.050 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:09.67 +41:33:21.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:09.67 +41:33:21.3: 15.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 22:02:21.09 +39:30:31.7
90.80789 -12.59165 galactic Lac Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1956169415041419264 | 22:02:18.13 +39:30:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:21.09 +39:30:31.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:21.09 +39:30:31.7: 15.15 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956169415041419264,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956169415041419264 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.66 21:51:39.74 +34:33:53.1
85.88650 -15.07266 galactic Peg Second-epoch detections are separated by 1.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:51:39.74 +34:33:53.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.74 +34:33:53.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.74 +34:33:53.1: 15.06 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:27:15.70 +41:14:43.5
86.84888 -6.89799 galactic Cyg Second-epoch detections are separated by 3.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:15.70 +41:14:43.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:15.70 +41:14:43.5: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:15.70 +41:14:43.5: 14.54 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 22:08:05.92 +41:53:33.1
93.16625 -11.34837 galactic Lac Second-epoch detections are separated by 0.6" and 3.2 pix
The object was found in VSX 9" ZTF J220806.43+415340.2
Type: EW
# Max. Min./Amp. JD0 Period
17.111 g Y 0.534 g 2458272.97290 0.343266000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:05.92 +41:53:33.1: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:05.92 +41:53:33.1: 14.92 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J220806.43+415340.2,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J220806.43+415340.2 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 21:31:06.96 +36:30:53.1
84.06235 -10.81762 galactic Cyg Second-epoch detections are separated by 1.0" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.7654+36.5145 | 21:31:06.96 +36:30:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:06.96 +36:30:53.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:06.96 +36:30:53.1: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7654+36.5145,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7654+36.5145 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 21:58:23.08 +40:16:07.5
90.67634 -11.52396 galactic Lac Second-epoch detections are separated by 1.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:23.08 +40:16:07.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.400+/-0.057 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:23.08 +40:16:07.5: 12.88 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:23.08 +40:16:07.5: 15.24 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.49 21:56:24.88 +33:43:30.6
86.10232 -16.34880 galactic Peg Second-epoch detections are separated by 1.7" and 3.6 pix
The object was found in VSX19" Gaia DR3 1947916210185665920
Type: ROT
# Max. Min./Amp. JD0 Period
17.070 G 17.100 G 0.317966000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:24.88 +33:43:30.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:24.88 +33:43:30.6: 14.84 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947916210185665920,2461185.8480,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947916210185665920 20260525.3480 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:37:56.98 +36:43:05.2
85.22049 -11.61204 galactic Cyg Second-epoch detections are separated by 1.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.4832+36.7302 | 21:37:53.50 +36:43:18.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:56.98 +36:43:05.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:56.98 +36:43:05.2: 14.74 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.4832+36.7302,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.4832+36.7302 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.67 21:54:34.88 +35:47:37.9
87.17874 -14.51993 galactic Peg Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:34.88 +35:47:37.9 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:34.88 +35:47:37.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:34.88 +35:47:37.9: 15.13 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.23 21:37:46.82 +38:52:30.6
86.68330 -10.00282 galactic Cyg Second-epoch detections are separated by 1.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:46.82 +38:52:30.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:46.82 +38:52:30.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:46.82 +38:52:30.6: 14.49 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:56:28.84 +40:10:13.7
90.32420 -11.37348 galactic Cyg Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1202+40.1728 | 21:56:28.84 +40:10:13.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.517+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:28.84 +40:10:13.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:28.84 +40:10:13.7: 14.91 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1202+40.1728,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1202+40.1728 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 22:07:18.00 +39:07:48.0
91.35242 -13.47370 galactic Lac Second-epoch detections are separated by 1.9" and 3.1 pix
The object was found in VSX 4" Gaia DR3 1956278580229840640
Type: ROT
# Max. Min./Amp. JD0 Period
14.740 G 14.770 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:18.00 +39:07:48.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:18.00 +39:07:48.0: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956278580229840640,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956278580229840640 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:45:58.85 +39:55:47.4
88.59742 -10.26961 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was found in VSX 1" Gaia DR3 1954120926101711872
Type: ROT
# Max. Min./Amp. JD0 Period
14.530 G 14.550 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:58.85 +39:55:47.4: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:58.85 +39:55:47.4: 14.75 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954120926101711872,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954120926101711872 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 21:55:53.88 +37:45:12.7
88.67440 -13.17790 galactic Cyg Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9635+37.7496 | 21:55:53.88 +37:45:12.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:53.88 +37:45:12.7: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:53.88 +37:45:12.7: 15.14 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.9635+37.7496,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9635+37.7496 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:33:42.50 +33:41:49.3
82.45116 -13.21293 galactic Cyg Second-epoch detections are separated by 0.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:33:42.50 +33:41:49.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:42.50 +33:41:49.3: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:42.50 +33:41:49.3: 14.90 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:34:53.25 +33:57:00.7
82.81272 -13.20008 galactic Cyg Second-epoch detections are separated by 1.8" and 4.0 pix
The object was found in VSX 2" Gaia DR3 1950271123576024576
Type: ROT
# Max. Min./Amp. JD0 Period
14.620 G 14.650 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:53.25 +33:57:00.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:53.25 +33:57:00.7: 15.24 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950271123576024576,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950271123576024576 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 22:01:30.88 +34:42:16.9
87.59883 -16.25940 galactic Peg Second-epoch detections are separated by 1.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:30.88 +34:42:16.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:30.88 +34:42:16.9: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:30.88 +34:42:16.9: 15.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 21:39:15.46 +34:56:58.7
84.18984 -13.08994 galactic Cyg Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:15.46 +34:56:58.7 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:15.46 +34:56:58.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:15.46 +34:56:58.7: 14.82 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.50 21:42:21.25 +38:13:06.7
86.90948 -11.08978 galactic Cyg Second-epoch detections are separated by 2.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5860+38.2161 | 21:42:21.25 +38:13:06.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:21.25 +38:13:06.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:21.25 +38:13:06.7: 14.96 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5860+38.2161,2461185.8480,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5860+38.2161 20260525.3480 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:42:57.35 +37:28:41.7
86.49680 -11.72103 galactic Cyg Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7449+37.4812 | 21:42:57.35 +37:28:41.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.307+/-0.043 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:57.35 +37:28:41.7: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:57.35 +37:28:41.7: 15.08 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.7449+37.4812,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7449+37.4812 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.29 21:31:22.22 +35:13:15.7
83.18217 -11.78273 galactic Cyg Second-epoch detections are separated by 2.6" and 4.2 pix
The object was found in VSX 3" Gaia DR3 1951335450830717056
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.530 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:22.22 +35:13:15.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:22.22 +35:13:15.7: 14.89 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951335450830717056,2461185.8480,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951335450830717056 20260525.3480 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:54:19.90 +38:01:39.8
88.60829 -12.76981 galactic Cyg Second-epoch detections are separated by 1.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:19.90 +38:01:39.8 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:19.90 +38:01:39.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:19.90 +38:01:39.8: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 21:53:53.39 +38:35:29.4
88.90779 -12.28004 galactic Cyg Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:53:53.39 +38:35:29.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:53.39 +38:35:29.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:53.39 +38:35:29.4: 14.47 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 22:03:34.20 +42:00:34.8
92.55129 -10.74970 galactic Lac Second-epoch detections are separated by 2.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.8932+42.0077 | 22:03:34.20 +42:00:34.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:34.20 +42:00:34.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:34.20 +42:00:34.8: 14.68 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.8932+42.0077,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.8932+42.0077 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 22:09:18.89 +39:53:05.4
92.13596 -13.10047 galactic Lac Second-epoch detections are separated by 0.6" and 3.3 pix
The object was found in VSX 2" Gaia DR3 1956415675587192704
Type: ROT
# Max. Min./Amp. JD0 Period
14.550 G 14.590 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:18.89 +39:53:05.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:18.89 +39:53:05.4: 15.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956415675587192704,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956415675587192704 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:37:25.90 +37:09:17.8
85.44576 -11.22117 galactic Cyg Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:25.90 +37:09:17.8 (user input) | T | P | (position from user input) J-Ks=0.745+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:25.90 +37:09:17.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:25.90 +37:09:17.8: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.63 22:06:27.14 +39:09:53.4
91.23906 -13.34696 galactic Lac Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:06:27.14 +39:09:53.4 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:27.14 +39:09:53.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:27.14 +39:09:53.4: 15.40 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:59:50.31 +38:00:40.6
89.46244 -13.46592 galactic Lac Second-epoch detections are separated by 2.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955783555179086592 | 21:59:52.41 +38:00:58.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:50.31 +38:00:40.6: 12.92 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:50.31 +38:00:40.6: 14.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955783555179086592,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955783555179086592 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 21:44:37.99 +36:48:09.0
86.29287 -12.44808 galactic Cyg Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:37.99 +36:48:09.0 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:37.99 +36:48:09.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:37.99 +36:48:09.0: 15.19 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:55:20.50 +36:22:54.1
87.68864 -14.16625 galactic Peg Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:55:20.50 +36:22:54.1 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:20.50 +36:22:54.1: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:20.50 +36:22:54.1: 14.72 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:47:08.02 +39:07:42.4
88.23541 -11.02132 galactic Cyg Second-epoch detections are separated by 2.6" and 3.2 pix
The object was found in VSX22" Gaia DR3 1953285022384759936
Type: ROT
# Max. Min./Amp. JD0 Period
16.750 G 16.790 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:08.02 +39:07:42.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:08.02 +39:07:42.4: 14.80 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953285022384759936,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953285022384759936 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.62 21:56:44.92 +37:19:57.3
88.53470 -13.61051 galactic Cyg Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.1700+37.3366 | 21:56:42.27 +37:20:11.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.752+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:44.92 +37:19:57.3: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:44.92 +37:19:57.3: 14.51 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1700+37.3366,2461185.8480,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1700+37.3366 20260525.3480 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 21:36:01.16 +35:40:54.0
84.20700 -12.10406 galactic Cyg Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:01.16 +35:40:54.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:01.16 +35:40:54.0: 12.88 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:01.16 +35:40:54.0: 14.73 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.51 22:11:07.90 +41:18:47.3
93.28485 -12.15067 galactic Lac Second-epoch detections are separated by 0.7" and 3.4 pix
The object was found in VSX 7" Gaia DR3 1958231072358590208
Type: S
# Max. Min./Amp. JD0 Period
15.460 G 16.190 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:07.90 +41:18:47.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:07.90 +41:18:47.3: 15.09 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958231072358590208,2461185.8480,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958231072358590208 20260525.3480 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.38 21:35:51.51 +40:29:40.4
87.51852 -8.56071 galactic Cyg Second-epoch detections are separated by 4.9" and 4.4 pix
The object was found in VSX13" NSV 13804
Type:
# Max. Min./Amp. JD0 Period
15.200 pg 16.200 pg
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:51.51 +40:29:40.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:51.51 +40:29:40.4: 14.63 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 13804,2461185.8480,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 13804 20260525.3480 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:50:22.16 +36:49:02.3
87.19115 -13.19052 galactic Cyg Second-epoch detections are separated by 1.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:50:22.16 +36:49:02.3 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:22.16 +36:49:02.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:22.16 +36:49:02.3: 15.14 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.44 22:00:11.33 +39:37:40.3
90.54688 -12.24107 galactic Lac Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:00:11.33 +39:37:40.3 (user input) | T | P | (position from user input) J-Ks=1.010+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:11.33 +39:37:40.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:11.33 +39:37:40.3: 14.85 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.41 21:49:30.71 +36:39:36.7
86.95216 -13.19807 galactic Cyg Second-epoch detections are separated by 1.4" and 3.6 pix
The object was found in VSX 2" Gaia DR3 1949455870062345088
Type: ROT
# Max. Min./Amp. JD0 Period
15.200 G 15.230 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:30.71 +36:39:36.7: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:30.71 +36:39:36.7: 15.02 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949455870062345088,2461185.8480,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949455870062345088 20260525.3480 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:40:16.32 +42:12:47.5
89.30487 -7.84415 galactic Cyg Second-epoch detections are separated by 1.2" and 3.6 pix
The object was found in VSX24" ZTF J214016.25+421311.1
Type: EW
# Max. Min./Amp. JD0 Period
17.551 r Y 0.622 r 2458601.99330 0.270542800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:16.32 +42:12:47.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:16.32 +42:12:47.5: 14.77 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214016.25+421311.1,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214016.25+421311.1 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.51 21:36:08.70 +34:46:10.3
83.58518 -12.78520 galactic Cyg Second-epoch detections are separated by 5.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:08.70 +34:46:10.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.384+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:08.70 +34:46:10.3: 13.51 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:08.70 +34:46:10.3: 14.91 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:49:05.03 +37:22:33.2
87.36411 -12.59951 galactic Cyg Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:49:05.03 +37:22:33.2 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:05.03 +37:22:33.2: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:05.03 +37:22:33.2: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 22:04:19.66 +41:12:36.0
92.17280 -11.47192 galactic Lac Second-epoch detections are separated by 2.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.0849+41.2111 | 22:04:20.57 +41:13:15.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:19.66 +41:12:36.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:19.66 +41:12:36.0: 14.58 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.0849+41.2111,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.0849+41.2111 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:44:48.48 +37:00:33.6
86.46003 -12.31639 galactic Cyg Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1891+37.0080 | 21:44:48.48 +37:00:33.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.454+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:48.48 +37:00:33.6: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:48.48 +37:00:33.6: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1891+37.0080,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1891+37.0080 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.67 21:48:10.19 +38:13:39.2
87.79195 -11.83591 galactic Cyg Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:48:10.19 +38:13:39.2 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:10.19 +38:13:39.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:10.19 +38:13:39.2: 15.19 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 21:32:50.72 +33:42:55.1
82.33176 -13.07499 galactic Cyg Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:50.72 +33:42:55.1 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:50.72 +33:42:55.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:50.72 +33:42:55.1: 15.11 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:59:59.41 +38:04:06.0
89.52299 -13.43987 galactic Lac Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:59:59.41 +38:04:06.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:59.41 +38:04:06.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:59.41 +38:04:06.0: 15.55 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.55 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.62 21:50:48.59 +40:31:54.5
89.70746 -10.40857 galactic Cyg Second-epoch detections are separated by 1.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.7150+40.5314 | 21:50:48.59 +40:31:54.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.716+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:48.59 +40:31:54.5: 13.27 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:48.59 +40:31:54.5: 14.84 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.7150+40.5314,2461185.8480,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.7150+40.5314 20260525.3480 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.33 21:38:19.67 +39:47:35.5
87.39089 -9.39659 galactic Cyg Second-epoch detections are separated by 2.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.5932+39.7857 | 21:38:19.67 +39:47:35.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.400+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:19.67 +39:47:35.5: 13.43 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.67 +39:47:35.5: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.5932+39.7857,2461185.8480,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5932+39.7857 20260525.3480 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:34:44.21 +34:15:39.7
83.01015 -12.95390 galactic Cyg Second-epoch detections are separated by 0.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:44.21 +34:15:39.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:44.21 +34:15:39.7: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:44.21 +34:15:39.7: 14.93 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:40:26.00 +37:35:59.3
86.20046 -11.29617 galactic Cyg Second-epoch detections are separated by 2.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0973+37.5949 | 21:40:26.00 +37:35:59.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.654+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:26.00 +37:35:59.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:26.00 +37:35:59.3: 14.89 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0973+37.5949,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0973+37.5949 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:31:05.39 +36:09:34.8
83.80705 -11.06918 galactic Cyg Second-epoch detections are separated by 2.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:05.39 +36:09:34.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:05.39 +36:09:34.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:05.39 +36:09:34.8: 14.83 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.30 21:29:09.98 +41:18:07.3
87.14779 -7.10598 galactic Cyg Second-epoch detections are separated by 1.4" and 3.8 pix
The object was found in VSX 2" Gaia DR3 1967015276919609216
Type: VAR
# Max. Min./Amp. JD0 Period
14.520 G 14.530 G 0.014751500000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:09.98 +41:18:07.3: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:09.98 +41:18:07.3: 14.51 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1967015276919609216,2461185.8480,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967015276919609216 20260525.3480 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:45:06.46 +36:34:14.0
86.20828 -12.68479 galactic Cyg Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:06.46 +36:34:14.0 (user input) | T | P | (position from user input) J-Ks=0.511+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:06.46 +36:34:14.0: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:06.46 +36:34:14.0: 14.88 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:58:27.13 +41:39:26.3
91.56527 -10.44379 galactic Lac Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.6163+41.6662 | 21:58:27.13 +41:39:26.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.795+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:27.13 +41:39:26.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:27.13 +41:39:26.3: 14.77 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.6163+41.6662,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.6163+41.6662 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.27 21:26:40.62 +35:39:06.4
82.79532 -10.80522 galactic Cyg Second-epoch detections are separated by 6.9" and 4.2 pix
The object was found in VSX 7" Gaia DR3 1951509860864029440
Type: ROT
# Max. Min./Amp. JD0 Period
14.770 G 14.800 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:40.62 +35:39:06.4: 13.26 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:40.62 +35:39:06.4: 14.57 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951509860864029440,2461185.8480,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951509860864029440 20260525.3480 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.68 21:54:14.47 +37:16:15.6
88.09857 -13.34113 galactic Cyg Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:14.47 +37:16:15.6 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:14.47 +37:16:15.6: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:14.47 +37:16:15.6: 15.11 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:51:58.13 +41:43:01.2
90.64725 -9.63664 galactic Cyg Second-epoch detections are separated by 2.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.9971+41.7274 | 21:51:58.13 +41:43:01.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.629+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:58.13 +41:43:01.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:58.13 +41:43:01.2: 14.97 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.9971+41.7274,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.9971+41.7274 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.34 21:45:18.35 +34:36:18.0
84.89657 -14.18058 galactic Cyg Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:18.35 +34:36:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:18.35 +34:36:18.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:18.35 +34:36:18.0: 15.18 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.63 21:41:54.81 +36:47:08.4
85.86601 -12.09770 galactic Cyg Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:54.81 +36:47:08.4 (user input) | T | P | (position from user input) J-Ks=0.000+/-0.084 (A)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:54.81 +36:47:08.4: 13.32 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:54.81 +36:47:08.4: 14.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.57 21:29:55.69 +35:17:01.3
83.01161 -11.53231 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was found in VSX21" Gaia DR3 1951347682897773440
Type: E
# Max. Min./Amp. JD0 Period
17.160 G 17.520 G 0.285046000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:55.69 +35:17:01.3: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:55.69 +35:17:01.3: 14.52 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951347682897773440,2461185.8480,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951347682897773440 20260525.3480 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 21:45:41.62 +35:36:34.3
85.64525 -13.48281 galactic Cyg Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:41.62 +35:36:34.3 (user input) | T | P | (position from user input) J-Ks=0.289+/-0.043 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:41.62 +35:36:34.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:41.62 +35:36:34.3: 15.31 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.51 21:37:36.08 +34:52:16.3
83.87993 -12.91594 galactic Cyg Second-epoch detections are separated by 2.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:36.08 +34:52:16.3 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:36.08 +34:52:16.3: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:36.08 +34:52:16.3: 15.14 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.37 21:35:22.68 +38:34:23.9
86.12596 -9.90629 galactic Cyg Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.8476+38.5796 | 21:35:22.68 +38:34:23.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:22.68 +38:34:23.9: 13.22 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:22.68 +38:34:23.9: 14.88 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8476+38.5796,2461185.8480,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8476+38.5796 20260525.3480 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:43:00.86 +35:26:44.6
85.11533 -13.24159 galactic Cyg Second-epoch detections are separated by 2.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:00.86 +35:26:44.6 (user input) | T | P | (position from user input) J-Ks=0.513+/-0.049 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:00.86 +35:26:44.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:00.86 +35:26:44.6: 15.02 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.51 21:46:40.74 +34:44:02.8
85.20275 -14.27170 galactic Cyg Second-epoch detections are separated by 2.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:46:40.74 +34:44:02.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:40.74 +34:44:02.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:40.74 +34:44:02.8: 15.03 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:42:17.53 +34:59:16.4
84.68712 -13.48200 galactic Cyg Second-epoch detections are separated by 1.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:17.53 +34:59:16.4 (user input) | T | P | (position from user input) J-Ks=0.516+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:17.53 +34:59:16.4: 12.87 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:17.53 +34:59:16.4: 15.22 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.61 21:54:33.27 +39:45:07.3
89.76278 -11.46556 galactic Cyg Second-epoch detections are separated by 0.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:54:33.27 +39:45:07.3 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:33.27 +39:45:07.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:33.27 +39:45:07.3: 14.94 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:35:57.20 +34:28:48.1
83.35167 -12.96835 galactic Cyg Second-epoch detections are separated by 3.9" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:57.20 +34:28:48.1 (user input) | T | P | (position from user input) J-Ks=0.607+/- (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:57.20 +34:28:48.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:57.20 +34:28:48.1: 15.35 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:52:02.06 +38:59:15.3
88.88229 -11.74433 galactic Cyg Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.0188+38.9971 | 21:52:02.06 +38:59:15.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.711+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:02.06 +38:59:15.3: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:02.06 +38:59:15.3: 14.76 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J328.0188+38.9971,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.0188+38.9971 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 21:32:42.44 +36:55:39.2
84.58757 -10.74087 galactic Cyg Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:42.44 +36:55:39.2 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:42.44 +36:55:39.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:42.44 +36:55:39.2: 15.05 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.45 21:58:13.02 +41:37:34.2
91.51059 -10.44096 galactic Lac Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:58:13.02 +41:37:34.2 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:13.02 +41:37:34.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:13.02 +41:37:34.2: 15.32 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:30:51.48 +34:08:40.4
82.33631 -12.47987 galactic Cyg Second-epoch detections are separated by 5.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.7158+34.1425 | 21:30:51.48 +34:08:40.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.382+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:51.48 +34:08:40.4: 13.37 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:51.48 +34:08:40.4: 15.04 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7158+34.1425,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7158+34.1425 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.54 21:43:08.02 +37:05:00.7
86.25504 -12.03896 galactic Cyg Second-epoch detections are separated by 1.2" and 3.7 pix
The object was found in VSX 0" Gaia DR3 1952645484575159040
Type: ROT
# Max. Min./Amp. JD0 Period
15.120 G 15.150 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:08.02 +37:05:00.7: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:08.02 +37:05:00.7: 15.04 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952645484575159040,2461185.8480,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952645484575159040 20260525.3480 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.46 21:32:03.99 +37:14:51.8
84.71872 -10.42115 galactic Cyg Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.0168+37.2479 | 21:32:03.99 +37:14:51.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.741+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:03.99 +37:14:51.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:03.99 +37:14:51.8: 14.61 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.0168+37.2479,2461185.8480,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.0168+37.2479 20260525.3480 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.51 21:47:40.00 +41:28:28.3
89.86444 -9.30565 galactic Cyg Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:47:40.00 +41:28:28.3 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:40.00 +41:28:28.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:40.00 +41:28:28.3: 14.92 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.59 21:41:56.96 +38:01:50.7
86.72139 -11.17662 galactic Cyg Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953578484609640320 | 21:41:58.07 +38:01:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.596+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:56.96 +38:01:50.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:56.96 +38:01:50.7: 15.39 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.39 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953578484609640320,2461185.8480,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953578484609640320 20260525.3480 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.65 21:42:08.11 +39:54:00.0
88.01441 -9.80584 galactic Cyg Second-epoch detections are separated by 3.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:08.11 +39:54:00.0 (user input) | T | P | (position from user input) J-Ks=0.476+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:08.11 +39:54:00.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:08.11 +39:54:00.0: 15.55 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.55 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.57 21:28:54.95 +36:35:23.5
83.79338 -10.45568 galactic Cyg Second-epoch detections are separated by 2.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:54.95 +36:35:23.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:54.95 +36:35:23.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:54.95 +36:35:23.5: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.36 21:29:37.24 +34:35:10.8
82.46662 -11.98575 galactic Cyg Second-epoch detections are separated by 0.4" and 4.0 pix
The object was found in VSX 2" Gaia DR3 1950469035671582336
Type: ROT
# Max. Min./Amp. JD0 Period
14.480 G 14.500 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:37.24 +34:35:10.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:37.24 +34:35:10.8: 14.80 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950469035671582336,2461185.8480,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950469035671582336 20260525.3480 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.52 21:43:20.90 +38:08:13.2
87.00294 -11.28060 galactic Cyg Second-epoch detections are separated by 2.5" and 3.6 pix
The object was found in VSX 2" Gaia DR3 1952834841094071680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.150 G 15.200 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:20.90 +38:08:13.2: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:20.90 +38:08:13.2: 14.90 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952834841094071680,2461185.8480,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952834841094071680 20260525.3480 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.56 21:27:23.67 +37:00:28.1
83.87037 -9.94413 galactic Cyg Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:23.67 +37:00:28.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:23.67 +37:00:28.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:23.67 +37:00:28.1: 14.86 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.32 21:35:04.43 +35:48:29.8
84.15322 -11.88030 galactic Cyg Second-epoch detections are separated by 2.5" and 3.6 pix
The object was found in VSX 2" Gaia DR3 1951001749052505088
Type: ROT
# Max. Min./Amp. JD0 Period
14.450 G 14.490 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:04.43 +35:48:29.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:04.43 +35:48:29.8: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951001749052505088,2461185.8480,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951001749052505088 20260525.3480 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.47 21:42:08.14 +41:34:23.5
89.13795 -8.55308 galactic Cyg Second-epoch detections are separated by 0.5" and 3.4 pix
The object was found in VSX 1" Gaia DR3 1966553344594875776
Type: VAR
# Max. Min./Amp. JD0 Period
14.820 G 14.930 G 0.091458300000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:08.14 +41:34:23.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:08.14 +41:34:23.5: 14.68 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966553344594875776,2461185.8480,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966553344594875776 20260525.3480 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.55 21:39:13.02 +38:06:35.0
86.36902 -10.75739 galactic Cyg Second-epoch detections are separated by 1.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1953547045448977280 | 21:39:16.70 +38:06:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.563+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:13.02 +38:06:35.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:13.02 +38:06:35.0: 15.13 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953547045448977280,2461185.8480,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953547045448977280 20260525.3480 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.39 21:27:01.23 +34:53:28.2
82.29843 -11.39318 galactic Cyg Second-epoch detections are separated by 1.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.7590+34.9027 | 21:27:01.23 +34:53:28.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.434+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:01.23 +34:53:28.2: 13.03 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:01.23 +34:53:28.2: 14.76 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.7590+34.9027,2461185.8480,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.7590+34.9027 20260525.3480 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.43 21:27:08.97 +35:52:28.6
83.02447 -10.71486 galactic Cyg Second-epoch detections are separated by 1.2" and 3.6 pix
The object was found in VSX 1" Gaia DR3 1951530717225138816
Type: ROT
# Max. Min./Amp. JD0 Period
14.560 G 14.590 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:08.97 +35:52:28.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:08.97 +35:52:28.6: 14.37 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951530717225138816,2461185.8480,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951530717225138816 20260525.3480 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.48 21:32:03.16 +35:39:41.6
83.59699 -11.56284 galactic Cyg Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:32:03.16 +35:39:41.6 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:03.16 +35:39:41.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:03.16 +35:39:41.6: 14.97 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 12.53 21:30:23.75 +40:32:52.1
86.79075 -7.81129 galactic Cyg Second-epoch detections are separated by 2.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:23.75 +40:32:52.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.776+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:23.75 +40:32:52.1: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:23.75 +40:32:52.1: 14.70 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8480,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3480 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.24 21:18:30.76 +41:07:56.6
85.59717 -5.81429 galactic Cyg Second-epoch detections are separated by 3.2" and 3.3 pix
The object was found in VSX 3" V0531 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.900 pg < 16.500 pg 2428045.00000 257.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:30.76 +41:07:56.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:30.76 +41:07:56.6: 13.87 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0531 Cyg,2461185.8480,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0531 Cyg 20260525.3480 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3480 2461185.8480 10.13 21:26:52.42 +41:39:00.1
87.08052 -6.55730 galactic Cyg Second-epoch detections are separated by 0.8" and 3.8 pix
The object was found in VSX 4" V0607 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.300 pg < 16.300 pg 2433510.00000 130.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:52.42 +41:39:00.1: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:52.42 +41:39:00.1: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0607 Cyg,2461185.8480,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0607 Cyg 20260525.3480 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461185.84821014 25.05.2026 08:21:15.356 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 19865
Objects passed selection criteria: 19858
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 18935.2
Average stars matched: 16816.8 (88.8119 %)
Memory usage VmPeak: 126116 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 05:50:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461185.84821014 25.05.2026 08:21:15.356 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 997
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 205 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 146541
Objects passed selection criteria: 146129
Measurements per detected object (mean, median, min, max): 3.3 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 3.0 2 4
Average stars detected per image: 136822
Average stars matched: 122532 (89.556 %)
Memory usage VmPeak: 2090864 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 05:55:57 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461185.84774850
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (1st reference image)
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Image size: 932.3'x637.3' 15.5(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.99"/pix along the Y axis
Image center: 21:48:57.820 +38:02:09.57 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:06.616 +38:00:06.76 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:06.616 +38:00:06.76
Angular distance between the image centers 0.0447 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:05.176 +38:00:19.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:05.176 +38:00:19.58
Angular distance between the image centers 0.0389 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:49:06.616 +38:00:06.76
Second-epoch second image center 21:49:05.176 +38:00:19.58
Angular distance between the image centers 0.00592 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.9dzGuMXJEU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits &> /tmp/tmp.DlCrz6AikQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits &> /tmp/tmp.m0KOsZiSiu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits &> /tmp/tmp.ng9cVQSA5n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.968900
a=0.000000 b=1.000000 c=22.968900
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (aperture=6.2)
Read 21746 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5217 to 337.7622 deg, Dec +32.2988 to +43.2789 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.5217 to 337.7622 deg, Dec 32.2988 to 43.2789 deg
Loaded 21125 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 13298 out of 14228 total matches.
Matched with Tycho-2 14228 out of 21746 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits (aperture=7.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
2.5 pix fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
2.2 pix wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Limiting magnitude estimates:
15.2 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
14.7 mag. Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
14.9 mag. fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
14.9 mag. fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9dzGuMXJEU (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2960, passed=28429
Got 28429 stars (including 25433 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 28429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 424 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 377 matched stars entering correct_measured_positions(), 326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 373 matched stars entering correct_measured_positions(), 11634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 495 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 453 matched stars entering correct_measured_positions(), 11686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
Accuracy estimation diagnostic: 452 matched stars entering correct_measured_positions(), 13987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
Excluding outliers - 452 stars left (next iteration limit 410)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits N_match=452 sigma_overall_arcsec=5.245 sigma_q1_arcsec=26.359 sigma_q2_arcsec=5.045 sigma_q3_arcsec=33.611 sigma_q4_arcsec=3.580 n_q1=17 n_q2=196 n_q3=13 n_q4=226 worst_quadrant_to_overall_ratio=6.408
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DlCrz6AikQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1940, passed=21746
Got 21746 stars (including 19798 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
util/solve_plate_with_UCAC5 got 21746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits N_match=958 sigma_overall_arcsec=0.836 sigma_q1_arcsec=0.742 sigma_q2_arcsec=0.917 sigma_q3_arcsec=0.784 sigma_q4_arcsec=1.358 n_q1=279 n_q2=165 n_q3=306 n_q4=208 worst_quadrant_to_overall_ratio=1.625
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -region wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.m0KOsZiSiu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2022, passed=23277
Got 23277 stars (including 21229 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat
util/solve_plate_with_UCAC5 got 23277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits N_match=964 sigma_overall_arcsec=0.653 sigma_q1_arcsec=0.532 sigma_q2_arcsec=0.763 sigma_q3_arcsec=0.628 sigma_q4_arcsec=0.681 n_q1=229 n_q2=225 n_q3=271 n_q4=239 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ng9cVQSA5n (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2033, passed=23327
Got 23327 stars (including 21273 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat
util/solve_plate_with_UCAC5 got 23327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 22970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 22970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 22969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits N_match=966 sigma_overall_arcsec=0.670 sigma_q1_arcsec=0.558 sigma_q2_arcsec=0.733 sigma_q3_arcsec=0.633 sigma_q4_arcsec=0.777 n_q1=229 n_q2=218 n_q3=274 n_q4=245 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits sigma_overall=5.245 worst_q_ratio=6.408
ref2=Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits sigma_overall=0.836 worst_q_ratio=1.625
new1=fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits sigma_overall=0.653 worst_q_ratio=1.169
new2=fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits sigma_overall=0.670 worst_q_ratio=1.161
reference average sigma_overall=3.0405 worst_q_ratio=4.0165
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041_astrometric_residuals.png (452 matched stars from wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728_astrometric_residuals.png (958 matched stars from wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350_astrometric_residuals.png (964 matched stars from wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351_astrometric_residuals.png (966 matched stars from wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-20-35_20.00sec_4.90C_LIGHT_0350.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q2b1x1_033155_TTUQ2b1x1_2931158_LV7T5Czs/wcs_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:34.11 +39:25:49.7: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:48.59 +35:34:28.4: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:02.30 +33:43:20.4: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:16.18 +34:44:53.6: 12.55 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:03:26.69 +37:53:16.4: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:43.57 +38:06:43.0: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:34.11 +39:25:49.7: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry filter REJECTED candidate at 21:50:34.11 +39:25:49.7: ref_mag=12.16 +/- 0.02 new_mean_mag=12.1799 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:48.59 +35:34:28.4: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Forced photometry filter REJECTED candidate at 21:58:48.59 +35:34:28.4: ref_mag=12.47 +/- 0.02 new_mean_mag=12.2863 delta=0.18 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:27.66 +40:44:00.9: 15.25 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:15.00 +38:46:27.0: 14.44 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:02.30 +33:43:20.4: 11.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.02
Forced photometry filter REJECTED candidate at 22:10:02.30 +33:43:20.4: ref_mag=11.88 +/- 0.02 new_mean_mag=12.0883 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:16.18 +34:44:53.6: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 21:43:16.18 +34:44:53.6: ref_mag=12.41 +/- 0.01 new_mean_mag=12.2395 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:03:26.69 +37:53:16.4: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Forced photometry filter REJECTED candidate at 22:03:26.69 +37:53:16.4: ref_mag=12.39 +/- 0.02 new_mean_mag=12.2542 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:02.37 +39:36:17.1: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:43.57 +38:06:43.0: 12.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.02
Forced photometry filter REJECTED candidate at 21:37:43.57 +38:06:43.0: ref_mag=12.06 +/- 0.02 new_mean_mag=12.1327 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:37.64 +33:53:19.1: 15.50 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:27.66 +40:44:00.9: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter REJECTED candidate at 21:44:27.66 +40:44:00.9: ref_mag=12.28 +/- 0.02 new_mean_mag=12.2300 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:15.00 +38:46:27.0: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Forced photometry filter KEPT candidate at 21:31:15.00 +38:46:27.0: ref_mag=12.76 +/- 0.03 new_mean_mag=11.8113 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:02.37 +39:36:17.1: 12.14 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:37.64 +33:53:19.1: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Forced photometry filter REJECTED candidate at 21:51:02.37 +39:36:17.1: ref_mag=12.14 +/- 0.02 new_mean_mag=12.1327 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry filter REJECTED candidate at 21:55:37.64 +33:53:19.1: ref_mag=12.48 +/- 0.02 new_mean_mag=12.2864 delta=0.19 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:36.53 +42:10:28.2: 14.64 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:36.53 +42:10:28.2: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter REJECTED candidate at 21:42:36.53 +42:10:28.2: ref_mag=12.28 +/- 0.02 new_mean_mag=12.2732 delta=0.00 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out37936.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 37891_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37891_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37931_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37931_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:01:54.20 +36:57:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37936_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37936_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:31:15.00 +38:46:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 5.163 1964379403950450560 322.81239217790 +38.77559847284 12.1472 10.2801 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 37948_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37948_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37952_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37952_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37961_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37961_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37972_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37972_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37975_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37975_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37978_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37978_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37979_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37979_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 37980_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 37980_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 38006_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 38006_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253156_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253156_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253158_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253158_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253171_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253171_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253177_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253177_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253187_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253187_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253194_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253194_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253203_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253203_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253204_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253204_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253206_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253206_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253210_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253210_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253212_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253212_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253215_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253215_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253216_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253216_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253224_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253224_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253230_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253230_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253234_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253234_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253236_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253236_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253243_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253243_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253246_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253246_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253249_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253249_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253256_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253256_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253267_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253267_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:28:30.99 +38:22:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253273_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253273_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253276_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253276_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253277_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253277_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253279_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253279_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253284_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253284_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253288_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253288_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253289_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253289_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253295_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253295_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253303_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253303_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253306_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253306_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253315_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253315_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253326_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253326_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253327_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253327_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253329_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253329_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253332_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253332_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253335_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253335_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253338_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253338_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253341_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253341_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253344_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253344_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253345_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253345_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253353_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253353_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253354_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253354_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253363_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253363_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253367_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253367_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253368_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253368_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253379_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253379_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253380_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253380_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253381_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253381_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253389_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253389_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253390_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253390_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253395_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253395_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253397_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253397_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253408_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253408_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253409_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253409_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253429_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253429_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253432_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253432_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253446_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253446_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253447_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253447_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253450_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253450_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253451_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253451_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253458_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253458_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 253471_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253471_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253484_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253484_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253489_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253489_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253490_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253490_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253494_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253494_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253500_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253500_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253501_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253501_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253503_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253503_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253505_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253505_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253506_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253506_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253514_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253514_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253518_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253518_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253519_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253519_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253533_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253533_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253535_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253535_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253538_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253538_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253540_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253540_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253543_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253543_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253545_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253545_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253547_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253547_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253557_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253557_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253564_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253564_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253567_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253567_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253571_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253571_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253572_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253572_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253574_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253574_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253592_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253592_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253605_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253605_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253610_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253610_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253612_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253612_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253614_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253614_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253618_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253618_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253642_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253642_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253645_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253645_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253650_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253650_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253652_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253652_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 253678_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253678_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253687_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253687_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253690_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253690_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253702_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253702_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253704_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253704_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253710_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253710_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253733_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253733_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253745_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253745_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253752_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253752_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253754_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253754_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253759_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253759_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253778_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253778_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253780_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253780_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253799_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253799_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253801_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253801_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 253802_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253802_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253804_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253804_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253806_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253806_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253817_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253817_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253820_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253820_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253828_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253828_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253829_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253829_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253855_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253855_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253873_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253873_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253879_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253879_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253897_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253897_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253902_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253902_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253908_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253908_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253916_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253916_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253917_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253917_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253926_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253926_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253939_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253939_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253943_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253943_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253944_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253944_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253949_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253949_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253951_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 253951_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 253954_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253954_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253955_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253955_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253962_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253962_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253972_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253972_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253978_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253978_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 253994_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 253994_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254010_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254010_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254018_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254018_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254021_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254021_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254039_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254039_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254065_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254065_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254089_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254089_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254098_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254098_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254099_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254099_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254100_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254100_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254115_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254115_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254122_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254122_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:57:23.06 +40:56:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254126_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254126_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254145_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254145_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254155_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254155_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254172_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254172_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:01:57.44 +35:42:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254197_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254197_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254200_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254200_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:35:41.36 +36:47:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254207_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254207_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:08:02.77 +38:37:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254210_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254210_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254212_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254212_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254216_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254216_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:10:36.47 +41:28:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254225_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254225_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:58:37.27 +33:56:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254229_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254229_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:54:51.14 +40:08:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254238_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254238_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:42:55.39 +37:35:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254241_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254241_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254261_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254261_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254262_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254262_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254267_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254267_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254274_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254274_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254278_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254278_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254283_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254283_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 254309_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254309_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254312_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254312_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254316_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254316_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254321_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254321_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254323_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254323_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254337_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254337_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:41:19.45 +37:02:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254343_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254343_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254344_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254344_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254346_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254346_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254354_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254354_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254364_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254364_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254371_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254371_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:41:05.70 +41:56:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254380_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254380_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254381_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254381_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254382_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254382_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254383_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254383_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254388_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254388_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:05:08.10 +36:40:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254394_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254394_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254397_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254397_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254402_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254402_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254406_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254406_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254407_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254407_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:27:58.67 +34:36:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254411_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254411_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254414_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254414_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254450_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254450_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254452_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254452_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254470_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254470_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254471_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254471_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254473_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254473_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254474_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254474_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254479_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254479_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:56:08.77 +41:50:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254483_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254483_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254486_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254486_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254492_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254492_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254500_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254500_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:01:08.04 +39:15:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254512_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254512_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 254529_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254529_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:12:26.56 +40:55:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254536_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254536_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254564_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254564_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:08:28.90 +40:57:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254565_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254565_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:42:50.28 +37:29:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254578_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254578_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:47:14.39 +41:48:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254587_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254587_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254592_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254592_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 254597_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254597_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:56:49.81 +42:13:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254623_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254623_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254637_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254637_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:42:45.62 +36:52:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254655_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254655_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:56:37.97 +37:20:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254663_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254663_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254665_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254665_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:08:10.06 +37:08:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254671_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254671_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:38:32.97 +37:54:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254700_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254700_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254708_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254708_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 254709_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254709_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:10:04.81 +41:24:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254716_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254716_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:58:07.73 +38:56:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254718_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254718_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:57:40.57 +37:18:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254729_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254729_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:01:55.27 +35:25:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254732_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254732_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:02:03.96 +34:25:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254751_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254751_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254762_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254762_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254766_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254766_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:57:06.79 +34:35:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254774_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254774_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254777_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254777_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:10:39.75 +41:12:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254780_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254780_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:06:02.15 +38:41:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254784_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254784_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:42:46.49 +37:59:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254790_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254790_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:06:46.65 +39:39:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254795_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254795_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254797_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254797_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254799_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254799_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:00:54.64 +41:16:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254802_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254802_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254807_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254807_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 254813_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254813_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 254817_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254817_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:50:27.48 +35:49:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254826_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254826_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254835_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254835_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:04:00.09 +39:46:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254841_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254841_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:49:54.75 +34:54:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254844_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254844_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 254845_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254845_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:50:52.37 +39:37:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254847_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254847_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:05:15.67 +37:31:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254849_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254849_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:04:54.97 +37:38:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254862_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254862_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:09:21.07 +33:46:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254863_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254863_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:54:04.46 +37:39:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254867_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254867_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254871_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254871_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:51:54.97 +33:54:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254872_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254872_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:47:01.54 +35:15:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254876_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254876_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:31:28.89 +34:33:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254886_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254886_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:59:59.49 +37:35:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254908_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254908_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:55:07.39 +37:29:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254917_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254917_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254934_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254934_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254943_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254943_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254952_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254952_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:49:20.34 +35:39:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254953_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254953_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254962_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254962_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:42:17.05 +37:34:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254964_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254964_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254970_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254970_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254973_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254973_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:55:01.62 +42:15:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254975_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254975_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:44:49.87 +36:56:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254979_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254979_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 254984_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254984_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:50:11.61 +35:33:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254986_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 254986_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:58:15.55 +41:40:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254999_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 254999_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255007_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255007_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 255012_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255012_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:49:54.40 +37:45:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255013_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255013_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:09:23.83 +40:29:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255020_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255020_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255032_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255032_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 255033_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255033_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255040_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255040_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255044_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255044_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:00:00.23 +38:42:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255051_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255051_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:43:32.16 +38:44:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255055_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255055_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255067_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255067_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255076_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255076_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 255084_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255084_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255091_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255091_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255101_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255101_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255134_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255134_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255135_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255135_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255151_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255151_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:58:13.72 +38:26:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255152_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255152_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 255157_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255157_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 255167_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255167_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 255176_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255176_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:59:00.24 +41:56:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255223_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255223_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255229_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255229_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255268_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255268_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255270_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255270_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:49:46.93 +41:07:50.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255276_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255276_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:49:18.27 +39:21:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255281_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255281_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255287_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255287_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255293_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255293_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255295_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255295_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255303_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255303_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255309_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255309_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255339_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255339_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255361_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255361_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:04:37.00 +38:54:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255362_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255362_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 255377_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255377_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255393_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255393_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255396_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255396_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:43:03.36 +37:32:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255406_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255406_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255410_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255410_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255420_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255420_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 255433_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255433_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255495_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255495_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255501_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255501_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255513_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255513_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255518_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255518_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255535_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255535_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255539_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255539_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 255572_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255572_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255577_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255577_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:06:40.85 +39:16:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255580_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255580_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255583_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255583_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 255594_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255594_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255600_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255600_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255614_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255614_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255615_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255615_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:02:25.93 +38:25:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255621_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255621_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255624_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255624_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 255626_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255626_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:44:26.93 +39:22:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255641_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255641_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255652_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255652_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255659_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255659_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255683_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255683_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255688_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255688_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255722_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255722_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255728_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255728_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255750_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255750_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 255752_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255752_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255771_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255771_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255780_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255780_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255790_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255790_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255798_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255798_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255824_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255824_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 255854_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255854_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255873_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255873_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255884_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255884_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255887_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255887_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255890_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255890_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:46:08.84 +35:33:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255921_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255921_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255949_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255949_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 255959_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 255959_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 255960_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255960_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255976_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255976_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 255997_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 255997_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256032_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256032_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 256034_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256034_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 256049_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256049_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:41:51.04 +35:55:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256055_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256055_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256059_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256059_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 256102_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256102_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256118_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256118_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 256127_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256127_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256131_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256131_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256149_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256149_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256167_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256167_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256169_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256169_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256184_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256184_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256195_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256195_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256222_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256222_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256232_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256232_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256281_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256281_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256303_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256303_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256332_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256332_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256418_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256418_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256421_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256421_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256422_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256422_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256435_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256435_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256449_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256449_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256458_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256458_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 256483_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256483_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 256494_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256494_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256530_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256530_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256547_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256547_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 256569_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256569_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256679_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256679_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256689_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256689_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256694_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256694_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256720_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256720_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256731_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256731_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256739_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256739_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256764_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256764_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256805_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256805_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256815_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256815_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256823_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256823_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256837_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256837_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256870_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256870_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256906_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256906_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256929_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256929_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256954_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256954_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256959_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256959_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 256967_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 256967_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:46:14.58 +38:44:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256971_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 256971_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257008_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257008_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257061_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257061_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257091_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257091_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257118_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257118_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257128_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257128_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257175_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257175_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257192_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257192_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257196_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257196_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 257204_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257204_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257215_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257215_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257223_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257223_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257272_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257272_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257292_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257292_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257310_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257310_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257318_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257318_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257339_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257339_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257349_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257349_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257355_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257355_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257361_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257361_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257385_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257385_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257396_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257396_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257411_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257411_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257417_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257417_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257439_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257439_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 257459_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257459_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257473_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257473_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257494_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257494_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257513_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257513_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257541_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257541_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257550_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257550_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257568_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257568_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257576_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257576_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257578_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257578_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257600_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257600_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 257603_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257603_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257607_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257607_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 22:00:33.01 +39:39:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257620_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257620_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 257621_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257621_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257626_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257626_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257634_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257634_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257670_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257670_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 257678_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257678_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257711_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257711_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257715_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257715_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257734_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257734_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 257747_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257747_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257768_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257768_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257775_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257775_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257794_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257794_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257803_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257803_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257815_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257815_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257829_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257829_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257838_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257838_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257842_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257842_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
**** FOUND 21:46:28.89 +39:28:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257893_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257893_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257901_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257901_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257902_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257902_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257926_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257926_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257937_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257937_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257960_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257960_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257962_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257962_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257976_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257976_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257984_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 257984_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 257985_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257985_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 257990_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 257990_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258005_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258005_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258007_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258007_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258023_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258023_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258029_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258029_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258036_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258036_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258041_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258041_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258042_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258042_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 258046_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258046_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258073_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258073_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258074_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258074_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258075_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258075_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258096_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258096_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258106_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258106_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258132_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258132_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258154_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258154_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258164_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258164_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258168_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258168_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258169_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258169_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258172_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258172_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258184_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258184_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258201_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258201_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258206_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258206_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258231_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258231_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258233_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258233_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258244_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258244_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258249_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258249_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258253_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258253_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258255_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258255_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258259_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258259_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 258266_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258266_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258280_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258280_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258290_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258290_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258294_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258294_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258313_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258313_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258317_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258317_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258327_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258327_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 258329_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258329_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258340_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258340_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258359_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258359_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258360_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258360_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258368_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258368_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258379_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258379_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258390_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258390_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258392_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258392_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 258403_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258403_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258417_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258417_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258421_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258421_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258436_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258436_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258442_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258442_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258471_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258471_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258472_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258472_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258476_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258476_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258485_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258485_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258500_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258500_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258505_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258505_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258507_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258507_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258515_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258515_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258538_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258538_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258543_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258543_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258570_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258570_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258577_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258577_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258583_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258583_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258589_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258589_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258594_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258594_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258595_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258595_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258596_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258596_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258601_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258601_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258603_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258603_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258607_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258607_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258612_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258612_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258615_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258615_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258616_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258616_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258617_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258617_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258643_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258643_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258646_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258646_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258650_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258650_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258651_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258651_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258665_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258665_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258666_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258666_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258667_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258667_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258669_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258669_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258670_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258670_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258674_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258674_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258688_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258688_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258689_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258689_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258719_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258719_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258743_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258743_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258751_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258751_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258753_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 258753_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 258761_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258761_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258767_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258767_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258784_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258784_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258800_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258800_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258805_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258805_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258822_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258822_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258823_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258823_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258825_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258825_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258827_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258827_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258829_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258829_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258836_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258836_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258841_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258841_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258854_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258854_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258858_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258858_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258878_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258878_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258885_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258885_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258897_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258897_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258916_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258916_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258919_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258919_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258934_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258934_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258941_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258941_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258944_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258944_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258966_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258966_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258969_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258969_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258975_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258975_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258976_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258976_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 258982_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 258982_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259005_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259005_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259015_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259015_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259016_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259016_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259029_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259029_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259034_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259034_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259044_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259044_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259046_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259046_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259048_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259048_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259055_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259055_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259058_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259058_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259059_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259059_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259078_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259078_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259087_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259087_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259098_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259098_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259101_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259101_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259113_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259113_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259129_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259129_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259134_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259134_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259137_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259137_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259148_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259148_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259150_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259150_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259160_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259160_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 259162_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259162_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259170_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259170_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259171_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259171_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259195_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259195_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259199_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259199_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259203_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259203_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259208_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259208_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259214_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259214_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259232_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259232_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259233_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259233_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259247_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259247_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259249_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259249_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259259_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259259_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259262_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259262_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259266_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259266_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259272_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259272_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259281_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259281_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259292_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259292_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259307_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259315_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259315_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259319_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259319_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259321_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259321_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259328_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259328_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259340_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259340_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259346_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259346_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259350_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259350_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259354_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259354_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259368_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259368_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259379_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259379_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259388_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259388_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259391_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259391_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259393_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259393_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259422_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259422_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259431_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259431_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259433_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259433_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259453_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259453_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259456_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259456_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259461_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259461_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259464_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259464_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259466_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259466_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259472_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259472_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259475_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259475_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259477_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259477_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259484_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259484_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259489_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259489_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259493_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259493_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259502_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259502_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259517_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259529_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259529_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259543_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259543_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259553_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259553_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259566_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259566_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259568_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259568_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259573_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259573_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259580_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259580_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259582_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259582_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259591_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259591_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259598_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259598_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259601_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259601_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259603_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259603_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259618_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259618_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259627_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259627_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259646_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259646_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259647_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259647_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259648_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259648_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259654_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259655_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259655_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259656_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259656_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259659_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259659_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 259670_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259670_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259671_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259671_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259678_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259678_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259679_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259679_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259681_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259681_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259682_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259682_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259684_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259684_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259686_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259686_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259688_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259688_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259694_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259694_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259704_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259704_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259710_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259710_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259711_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259711_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259712_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259712_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259713_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259713_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259727_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259727_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259730_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259730_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259732_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259732_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259733_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259733_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259742_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259742_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259755_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259755_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259759_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259759_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259789_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259789_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259793_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259793_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259796_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259796_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259797_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259797_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259799_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259799_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259828_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259828_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259830_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259830_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 259832_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259832_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259846_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259846_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259847_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259847_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259860_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259860_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259862_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259862_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259880_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259880_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259884_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259884_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259886_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259886_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259898_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259898_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259900_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259900_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259901_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259901_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259903_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259903_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259913_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259913_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259914_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259914_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259918_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259918_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259929_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259929_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259931_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259931_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259933_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259933_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259934_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259934_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 259937_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259937_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259949_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259949_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259953_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 259953_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 259966_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259966_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259987_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259987_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 259999_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 259999_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260007_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260007_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260008_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260008_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260038_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260038_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260043_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260043_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260047_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260047_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260056_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 260056_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 260063_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260063_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260072_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260072_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260073_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260073_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260080_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 260080_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 260087_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260087_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260095_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260095_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260105_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260105_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260106_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 260106_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 260131_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 260131_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 260150_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260150_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260162_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260162_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260169_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260169_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260213_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260213_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260219_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260251_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260251_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260252_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260252_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260255_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260255_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260324_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260324_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260336_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260336_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260346_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260346_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260355_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260355_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260387_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260419_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260419_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260462_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260462_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260485_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 260485_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
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Considering the candidate 260524_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260524_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260542_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260542_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260550_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260550_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 260661_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 260661_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 243136_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 243136_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
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Considering the candidate 233608_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
The candidate 233608_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 33331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
Preparing report for the candidate 33331_fd_Cyg-07-Q2b1x1_2026-05-25_03-21-15_20.00sec_5.00C_LIGHT_0351
make_report_in_HTML.sh Phase 2 (HTML assembly): 36s
make_report_in_HTML.sh TOTAL: 1431s
Prepared the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
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21:43:24.22 +39:02:44.7
21:54:13.84 +42:03:14.7
22:03:45.58 +37:16:45.0
21:58:01.47 +38:57:27.0
21:49:19.26 +36:58:39.0
21:52:57.14 +41:56:24.0
21:59:54.31 +34:16:50.9
21:55:11.88 +36:28:56.0
22:01:30.08 +41:04:28.8
22:00:40.88 +34:40:45.0
21:28:15.82 +34:43:42.3
21:33:16.16 +41:46:48.3
22:00:20.90 +41:35:27.5
22:08:56.95 +41:29:27.8
21:58:48.24 +40:45:27.6
21:38:03.92 +38:03:50.8
21:48:31.78 +39:16:35.8
21:55:20.84 +34:39:46.5
21:42:21.52 +36:16:15.6
22:02:43.72 +35:30:17.9
21:34:31.83 +40:00:34.5
21:54:17.40 +36:52:10.6
21:37:03.51 +37:31:36.8
22:04:39.71 +37:04:27.3
21:57:38.67 +36:43:41.1
21:59:07.04 +37:35:41.8
21:29:05.04 +40:36:55.7
21:33:40.02 +33:37:46.0
21:33:43.05 +37:03:45.6
22:08:55.68 +38:16:52.9
21:53:51.27 +33:51:00.5
21:27:30.62 +35:18:41.9
21:51:39.59 +40:18:36.0
22:02:49.10 +35:57:04.6
21:37:17.02 +36:54:05.4
21:49:30.28 +38:28:52.1
21:28:43.48 +36:04:03.7
22:00:10.43 +38:33:13.9
22:11:52.66 +40:52:48.1
21:43:28.90 +37:46:48.1
21:34:28.42 +40:12:23.8
22:11:50.18 +39:03:26.3
22:03:00.73 +38:51:52.9
21:57:52.96 +34:06:45.3
21:49:13.72 +35:11:21.8
22:02:05.34 +37:22:23.9
21:57:21.27 +37:30:14.8
21:42:25.14 +35:54:12.6
21:48:39.22 +37:49:35.3
21:44:01.36 +38:56:13.3
21:34:10.50 +35:44:49.6
22:01:39.44 +34:45:27.5
22:00:37.79 +41:43:04.1
21:54:53.71 +41:04:43.2
21:29:44.17 +35:02:48.4
21:59:17.07 +35:39:25.5
21:41:58.03 +35:21:26.8
22:04:41.21 +40:20:51.2
22:00:13.59 +38:25:18.0
21:46:22.62 +36:17:37.7
21:36:08.38 +34:28:55.9
21:58:26.35 +42:12:16.4
21:35:23.86 +34:51:32.9
21:31:17.69 +33:40:29.1
22:04:51.38 +36:57:57.2
22:06:53.62 +39:49:46.3
21:33:24.09 +35:46:28.4
21:39:07.59 +35:00:10.2
22:12:09.67 +41:33:21.3
22:02:21.09 +39:30:31.7
21:51:39.74 +34:33:53.1
21:27:15.70 +41:14:43.5
22:08:05.92 +41:53:33.1
21:31:06.96 +36:30:53.1
21:58:23.08 +40:16:07.5
21:56:24.88 +33:43:30.6
21:37:56.98 +36:43:05.2
21:54:34.88 +35:47:37.9
21:37:46.82 +38:52:30.6
21:56:28.84 +40:10:13.7
22:07:18.00 +39:07:48.0
21:45:58.85 +39:55:47.4
21:55:53.88 +37:45:12.7
21:33:42.50 +33:41:49.3
21:34:53.25 +33:57:00.7
22:01:30.88 +34:42:16.9
21:39:15.46 +34:56:58.7
21:42:21.25 +38:13:06.7
21:42:57.35 +37:28:41.7
21:31:22.22 +35:13:15.7
21:54:19.90 +38:01:39.8
21:53:53.39 +38:35:29.4
22:03:34.20 +42:00:34.8
22:09:18.89 +39:53:05.4
21:37:25.90 +37:09:17.8
22:06:27.14 +39:09:53.4
21:59:50.31 +38:00:40.6
21:44:37.99 +36:48:09.0
21:55:20.50 +36:22:54.1
21:47:08.02 +39:07:42.4
21:56:44.92 +37:19:57.3
21:36:01.16 +35:40:54.0
22:11:07.90 +41:18:47.3
21:35:51.51 +40:29:40.4
21:50:22.16 +36:49:02.3
22:00:11.33 +39:37:40.3
21:49:30.71 +36:39:36.7
21:40:16.32 +42:12:47.5
21:36:08.70 +34:46:10.3
21:49:05.03 +37:22:33.2
22:04:19.66 +41:12:36.0
21:44:48.48 +37:00:33.6
21:48:10.19 +38:13:39.2
21:32:50.72 +33:42:55.1
21:59:59.41 +38:04:06.0
21:50:48.59 +40:31:54.5
21:38:19.67 +39:47:35.5
21:34:44.21 +34:15:39.7
21:40:26.00 +37:35:59.3
21:31:05.39 +36:09:34.8
21:29:09.98 +41:18:07.3
21:45:06.46 +36:34:14.0
21:58:27.13 +41:39:26.3
21:26:40.62 +35:39:06.4
21:54:14.47 +37:16:15.6
21:51:58.13 +41:43:01.2
21:45:18.35 +34:36:18.0
21:41:54.81 +36:47:08.4
21:29:55.69 +35:17:01.3
21:45:41.62 +35:36:34.3
21:37:36.08 +34:52:16.3
21:35:22.68 +38:34:23.9
21:43:00.86 +35:26:44.6
21:46:40.74 +34:44:02.8
21:42:17.53 +34:59:16.4
21:54:33.27 +39:45:07.3
21:35:57.20 +34:28:48.1
21:52:02.06 +38:59:15.3
21:32:42.44 +36:55:39.2
21:58:13.02 +41:37:34.2
21:30:51.48 +34:08:40.4
21:43:08.02 +37:05:00.7
21:32:03.99 +37:14:51.8
21:47:40.00 +41:28:28.3
21:41:56.96 +38:01:50.7
21:42:08.11 +39:54:00.0
21:28:54.95 +36:35:23.5
21:29:37.24 +34:35:10.8
21:43:20.90 +38:08:13.2
21:27:23.67 +37:00:28.1
21:35:04.43 +35:48:29.8
21:42:08.14 +41:34:23.5
21:39:13.02 +38:06:35.0
21:27:01.23 +34:53:28.2
21:27:08.97 +35:52:28.6
21:32:03.16 +35:39:41.6
21:30:23.75 +40:32:52.1
21:26:52.42 +41:39:00.1
########### Completed Cyg-07-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:36:11.19 +38:20:58.6
21:42:02.26 +37:42:53.1
21:40:31.53 +37:49:27.5
21:42:44.12 +39:07:51.7
21:31:17.47 +37:57:30.7
21:41:56.61 +38:52:29.8
21:40:17.04 +41:25:00.8
21:29:26.32 +37:55:00.9
21:56:23.29 +38:47:33.2
21:42:39.45 +37:40:34.5
21:39:10.96 +36:29:08.3
21:45:01.35 +40:16:55.6
21:29:04.98 +34:49:01.3
22:06:13.56 +41:38:26.9
21:36:57.17 +34:14:37.0
21:34:02.89 +36:28:38.6
21:50:37.07 +36:00:47.8
21:34:54.31 +35:45:43.1
21:33:31.70 +37:30:03.8
21:35:45.33 +33:50:35.9
21:49:28.07 +34:19:21.2
21:51:47.59 +36:45:22.7
21:43:20.61 +36:54:41.3
21:28:45.26 +36:42:07.2
21:36:54.42 +37:55:38.1
21:47:02.34 +36:41:21.7
21:36:56.43 +36:30:10.2
21:48:57.11 +38:28:35.3
21:54:36.22 +36:42:13.8
21:54:21.74 +42:02:06.9
22:07:53.03 +37:40:43.6
21:39:19.17 +36:37:29.1
21:39:17.12 +36:38:31.8
22:06:02.53 +38:59:35.1
21:37:14.59 +37:16:14.3
22:00:25.81 +37:57:32.4
21:58:37.95 +35:47:12.2
21:45:21.68 +37:55:18.5
21:45:48.52 +34:00:26.9
21:46:11.76 +36:11:01.7
21:37:28.91 +34:32:02.1
21:27:14.01 +34:30:08.1
21:37:12.18 +40:33:58.9
21:42:26.08 +37:18:12.6
21:53:31.29 +36:34:23.1
21:28:13.25 +40:35:50.7
21:54:04.90 +35:09:18.4
22:05:53.67 +41:23:38.0
21:57:44.02 +34:13:27.3
22:06:42.48 +40:57:13.5
21:45:30.42 +40:39:22.2
21:36:23.81 +37:21:33.7
22:01:48.10 +38:11:19.5
22:08:28.75 +34:30:21.8
21:49:19.52 +40:40:24.4
21:59:04.05 +35:55:55.0
21:32:18.87 +39:50:34.0
21:36:13.40 +36:37:41.9
22:06:41.13 +40:11:40.3
22:10:06.42 +35:55:00.5
21:57:21.05 +35:17:18.2
22:01:48.30 +39:56:07.0
21:58:11.17 +38:50:11.7
21:35:46.01 +36:23:43.6
22:09:10.00 +41:58:24.6
21:35:14.10 +35:46:26.8
21:53:18.52 +38:48:06.9
21:48:40.82 +41:58:41.0
21:53:07.93 +40:37:52.5
22:02:56.32 +40:46:06.8
22:00:26.34 +35:56:03.5
21:51:26.79 +38:24:24.2
21:41:11.94 +41:00:50.9
21:50:25.25 +38:28:29.4
22:03:02.51 +36:29:37.6
21:46:04.46 +34:31:28.8
22:00:22.58 +36:02:18.8
21:56:03.61 +38:29:55.7
21:28:12.79 +36:49:25.2
21:55:53.68 +42:08:36.5
21:31:19.68 +39:08:30.9
21:51:41.99 +34:07:03.5
21:44:02.27 +38:24:38.7
21:43:24.81 +37:27:40.2
21:41:57.73 +41:24:19.5
21:42:33.81 +41:45:50.4
22:07:12.31 +41:10:46.1
21:29:22.39 +34:26:40.6
21:32:31.05 +37:13:03.8
22:09:10.52 +33:47:36.6
22:03:26.52 +35:25:29.3
21:41:45.31 +37:40:53.2
21:29:18.14 +33:38:40.5
22:08:01.57 +35:58:26.1
22:00:45.78 +42:12:40.6
21:44:03.17 +37:47:35.8
21:57:12.31 +36:23:41.2
21:49:03.73 +39:29:38.9
22:03:46.20 +38:55:41.6
21:53:48.08 +40:18:26.1
21:45:02.97 +36:40:08.0
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21:34:49.80 +42:03:15.4
21:47:46.78 +37:36:30.0
21:29:00.32 +38:59:30.2
21:35:25.71 +40:25:30.5
21:27:28.02 +39:54:38.6
21:53:31.10 +33:46:49.4
21:50:38.82 +39:20:18.3
21:46:35.91 +37:00:51.7
21:28:06.42 +33:41:27.0
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22:05:32.49 +38:58:33.0
21:51:31.60 +37:29:39.0
21:50:30.82 +36:49:51.1
22:00:16.07 +41:05:52.9
21:29:46.34 +35:53:26.3
21:57:31.30 +38:48:28.0
21:44:09.01 +35:27:53.6
21:43:02.34 +34:00:48.1
21:32:45.10 +38:02:03.6
21:51:29.81 +37:52:05.2
21:42:51.49 +37:11:24.5
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21:42:39.00 +37:00:24.2
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21:40:15.60 +37:50:20.1
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22:10:57.04 +37:02:43.5
22:06:24.16 +38:41:47.2
21:26:26.98 +37:43:49.9
21:40:39.67 +36:27:52.9
21:55:19.69 +36:41:47.8
21:26:40.74 +39:52:49.0
21:43:23.84 +33:45:14.5
21:43:17.63 +38:29:48.8
22:03:38.17 +36:16:08.0
21:58:28.78 +40:10:17.0
21:57:14.45 +42:01:03.9
21:33:10.28 +41:39:56.3
21:28:22.15 +41:32:00.3
21:29:16.83 +34:43:07.0
22:04:23.77 +39:34:05.5
22:05:37.45 +38:57:41.0
21:54:38.60 +36:53:53.5
21:30:29.91 +39:49:30.6
21:48:12.58 +41:41:12.5
21:30:08.27 +37:30:28.0
21:45:30.14 +42:12:25.2
22:03:06.42 +40:42:37.9
21:44:13.05 +38:35:36.7
21:58:00.76 +37:39:30.9
21:28:31.47 +41:22:58.2
21:31:31.11 +41:31:49.7
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21:40:43.84 +37:22:59.4
21:40:26.40 +39:27:29.0
21:33:11.14 +39:46:10.4
22:02:11.40 +35:32:41.6
21:49:22.29 +41:57:46.4
21:57:39.33 +41:47:18.3
21:50:25.17 +35:00:16.6
21:30:28.13 +38:52:35.3
21:35:35.36 +35:59:26.5
21:34:37.63 +34:15:56.3
22:10:32.03 +41:45:05.9
22:11:02.23 +38:11:05.6
22:12:04.92 +39:17:50.0
21:40:56.14 +41:13:20.7
22:07:02.72 +41:57:30.8
21:44:09.61 +37:55:02.7
21:33:22.18 +38:02:28.7
22:05:39.89 +34:53:38.5
21:33:13.81 +37:12:44.0
21:59:20.91 +36:56:49.2
22:06:30.62 +34:18:24.6
21:59:59.23 +36:08:33.3
21:37:46.88 +36:44:34.4
21:28:09.30 +41:14:37.1
21:32:51.76 +35:15:25.9
21:56:52.31 +39:21:22.0
21:27:20.05 +35:46:48.2
21:28:11.99 +34:45:25.7
21:54:25.08 +39:39:28.0
21:30:32.04 +35:46:44.4
21:46:48.64 +36:53:20.3
21:38:15.46 +38:02:08.4
21:36:49.67 +39:45:20.6
22:06:56.78 +36:48:40.3
22:00:17.84 +38:06:34.9
21:59:06.43 +34:00:17.5
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21:34:29.38 +39:23:38.8
22:01:14.44 +38:33:47.4
21:31:14.97 +38:46:29.7
22:09:13.59 +39:15:46.5
21:44:42.94 +35:29:07.5
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21:43:06.26 +37:12:23.6
21:40:41.05 +36:19:20.5
22:02:42.11 +37:08:59.4
22:02:14.92 +34:37:08.3
22:02:42.57 +41:44:09.7
22:00:24.33 +35:58:53.7
22:03:19.33 +33:44:47.9
22:10:02.92 +36:44:11.9
21:49:08.07 +35:40:21.4
22:06:31.92 +34:33:33.0
21:54:12.72 +35:10:05.1
21:40:47.62 +37:32:56.2
22:09:46.32 +41:39:59.1
21:47:33.77 +37:22:55.8
21:33:58.57 +36:17:17.8
22:04:59.77 +39:57:17.5
21:48:15.82 +35:31:04.0
22:02:04.72 +37:45:26.3
21:54:39.47 +39:49:48.7
22:11:31.18 +40:27:17.9
22:05:42.70 +35:53:01.6
21:48:57.95 +37:42:52.3
21:58:42.71 +38:46:43.2
22:10:20.20 +38:44:20.8
21:58:43.33 +42:11:57.9
21:49:41.31 +37:43:29.6
21:51:57.64 +37:11:55.0
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21:59:40.08 +41:01:41.0
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22:11:43.30 +42:07:49.5
21:36:14.22 +40:15:40.1
21:33:15.00 +33:54:30.0
21:56:29.42 +36:52:34.4
21:59:28.83 +37:59:48.3
21:35:57.86 +41:51:55.7
22:09:11.66 +36:46:05.4
21:41:04.38 +37:16:08.3
21:58:52.18 +37:02:33.4
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21:51:03.60 +36:58:53.3
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21:47:12.13 +36:46:39.3
21:55:27.21 +41:39:30.1
21:46:37.68 +36:31:34.8
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21:57:35.09 +40:21:27.2
21:48:08.00 +39:26:18.8
21:59:05.04 +35:36:42.6
21:50:41.80 +36:02:33.6
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21:49:15.19 +35:18:21.5
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21:32:14.37 +37:49:10.6
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21:57:11.29 +40:23:42.7
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21:50:34.42 +37:11:03.5
21:59:31.05 +42:08:24.3
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21:37:13.77 +40:19:25.1
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21:46:54.04 +39:15:19.9
21:56:34.64 +37:00:25.7
21:59:09.95 +36:16:48.9
21:39:06.45 +37:40:27.9
21:59:27.03 +41:38:40.6
21:34:22.92 +34:51:23.4
22:05:37.91 +35:36:47.0
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21:47:32.63 +41:45:11.6
22:06:02.05 +40:00:16.4
21:48:47.80 +38:52:57.8
21:47:31.33 +37:36:09.6
21:35:24.09 +36:47:16.4
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21:50:58.78 +36:44:37.4
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21:50:08.02 +34:33:28.4
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21:44:51.80 +36:12:12.5
21:54:32.82 +35:25:31.7
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21:47:51.58 +40:21:48.5
21:40:34.69 +33:42:27.1
21:45:18.29 +37:39:34.8
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21:36:58.26 +37:51:36.1
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21:55:36.33 +35:51:32.4
21:54:51.04 +40:07:59.2
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21:49:28.23 +38:12:27.0
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22:11:07.90 +41:18:47.3
21:35:51.51 +40:29:40.4
21:50:22.16 +36:49:02.3
22:00:11.33 +39:37:40.3
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21:42:17.53 +34:59:16.4
21:54:33.27 +39:45:07.3
21:35:57.20 +34:28:48.1
21:52:02.06 +38:59:15.3
21:32:42.44 +36:55:39.2
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21:30:51.48 +34:08:40.4
21:43:08.02 +37:05:00.7
21:32:03.99 +37:14:51.8
21:47:40.00 +41:28:28.3
21:41:56.96 +38:01:50.7
21:42:08.11 +39:54:00.0
21:28:54.95 +36:35:23.5
21:29:37.24 +34:35:10.8
21:43:20.90 +38:08:13.2
21:27:23.67 +37:00:28.1
21:35:04.43 +35:48:29.8
21:42:08.14 +41:34:23.5
21:39:13.02 +38:06:35.0
21:27:01.23 +34:53:28.2
21:27:08.97 +35:52:28.6
21:32:03.16 +35:39:41.6
21:30:23.75 +40:32:52.1
21:18:30.76 +41:07:56.6
21:26:52.42 +41:39:00.1
###################################################################################
21:36:11.19 +38:20:58.6 -- not an asteroid (will add it to exclusion list)
21:42:02.26 +37:42:53.1 -- not an asteroid (will add it to exclusion list)
21:40:31.53 +37:49:27.5 -- not an asteroid (will add it to exclusion list)
21:42:44.12 +39:07:51.7 -- not an asteroid (will add it to exclusion list)
21:31:17.47 +37:57:30.7 -- not an asteroid (will add it to exclusion list)
21:41:56.61 +38:52:29.8 -- not an asteroid (will add it to exclusion list)
21:40:17.04 +41:25:00.8 -- not an asteroid (will add it to exclusion list)
21:29:26.32 +37:55:00.9 -- not an asteroid (will add it to exclusion list)
21:56:23.29 +38:47:33.2 -- not an asteroid (will add it to exclusion list)
21:42:39.45 +37:40:34.5 -- not an asteroid (will add it to exclusion list)
21:39:10.96 +36:29:08.3 -- not an asteroid (will add it to exclusion list)
21:45:01.35 +40:16:55.6 -- not an asteroid (will add it to exclusion list)
21:29:04.98 +34:49:01.3 -- not an asteroid (will add it to exclusion list)
22:06:13.56 +41:38:26.9 -- not an asteroid (will add it to exclusion list)
21:36:57.17 +34:14:37.0 -- not an asteroid (will add it to exclusion list)
21:34:02.89 +36:28:38.6 -- not an asteroid (will add it to exclusion list)
21:50:37.07 +36:00:47.8 -- not an asteroid (will add it to exclusion list)
21:34:54.31 +35:45:43.1 -- not an asteroid (will add it to exclusion list)
21:33:31.70 +37:30:03.8 -- not an asteroid (will add it to exclusion list)
21:35:45.33 +33:50:35.9 -- not an asteroid (will add it to exclusion list)
21:49:28.07 +34:19:21.2 -- not an asteroid (will add it to exclusion list)
21:51:47.59 +36:45:22.7 -- not an asteroid (will add it to exclusion list)
21:43:20.61 +36:54:41.3 -- not an asteroid (will add it to exclusion list)
21:28:45.26 +36:42:07.2 -- not an asteroid (will add it to exclusion list)
21:36:54.42 +37:55:38.1 -- not an asteroid (will add it to exclusion list)
21:47:02.34 +36:41:21.7 -- not an asteroid (will add it to exclusion list)
21:36:56.43 +36:30:10.2 -- not an asteroid (will add it to exclusion list)
21:48:57.11 +38:28:35.3 -- not an asteroid (will add it to exclusion list)
21:54:36.22 +36:42:13.8 -- not an asteroid (will add it to exclusion list)
21:54:21.74 +42:02:06.9 -- not an asteroid (will add it to exclusion list)
22:07:53.03 +37:40:43.6 -- not an asteroid (will add it to exclusion list)
21:39:19.17 +36:37:29.1 -- not an asteroid (will add it to exclusion list)
21:39:17.12 +36:38:31.8 -- not an asteroid (will add it to exclusion list)
22:06:02.53 +38:59:35.1 -- not an asteroid (will add it to exclusion list)
21:37:14.59 +37:16:14.3 -- not an asteroid (will add it to exclusion list)
22:00:25.81 +37:57:32.4 -- not an asteroid (will add it to exclusion list)
21:58:37.95 +35:47:12.2 -- not an asteroid (will add it to exclusion list)
21:45:21.68 +37:55:18.5 -- not an asteroid (will add it to exclusion list)
21:45:48.52 +34:00:26.9 -- not an asteroid (will add it to exclusion list)
21:46:11.76 +36:11:01.7 -- not an asteroid (will add it to exclusion list)
21:37:28.91 +34:32:02.1 -- not an asteroid (will add it to exclusion list)
21:27:14.01 +34:30:08.1 -- not an asteroid (will add it to exclusion list)
21:37:12.18 +40:33:58.9 -- not an asteroid (will add it to exclusion list)
21:42:26.08 +37:18:12.6 -- not an asteroid (will add it to exclusion list)
21:53:31.29 +36:34:23.1 -- not an asteroid (will add it to exclusion list)
21:28:13.25 +40:35:50.7 -- not an asteroid (will add it to exclusion list)
21:54:04.90 +35:09:18.4 -- not an asteroid (will add it to exclusion list)
22:05:53.67 +41:23:38.0 -- not an asteroid (will add it to exclusion list)
21:57:44.02 +34:13:27.3 -- not an asteroid (will add it to exclusion list)
22:06:42.48 +40:57:13.5 -- not an asteroid (will add it to exclusion list)
21:45:30.42 +40:39:22.2 -- not an asteroid (will add it to exclusion list)
21:36:23.81 +37:21:33.7 -- not an asteroid (will add it to exclusion list)
22:01:48.10 +38:11:19.5 -- not an asteroid (will add it to exclusion list)
22:08:28.75 +34:30:21.8 -- not an asteroid (will add it to exclusion list)
21:49:19.52 +40:40:24.4 -- not an asteroid (will add it to exclusion list)
21:59:04.05 +35:55:55.0 -- not an asteroid (will add it to exclusion list)
21:32:18.87 +39:50:34.0 -- not an asteroid (will add it to exclusion list)
21:36:13.40 +36:37:41.9 -- not an asteroid (will add it to exclusion list)
22:06:41.13 +40:11:40.3 -- not an asteroid (will add it to exclusion list)
22:10:06.42 +35:55:00.5 -- not an asteroid (will add it to exclusion list)
21:57:21.05 +35:17:18.2 -- not an asteroid (will add it to exclusion list)
22:01:48.30 +39:56:07.0 -- not an asteroid (will add it to exclusion list)
21:58:11.17 +38:50:11.7 -- not an asteroid (will add it to exclusion list)
21:35:46.01 +36:23:43.6 -- not an asteroid (will add it to exclusion list)
22:09:10.00 +41:58:24.6 -- not an asteroid (will add it to exclusion list)
21:35:14.10 +35:46:26.8 -- not an asteroid (will add it to exclusion list)
21:53:18.52 +38:48:06.9 -- not an asteroid (will add it to exclusion list)
21:48:40.82 +41:58:41.0 -- not an asteroid (will add it to exclusion list)
21:53:07.93 +40:37:52.5 -- not an asteroid (will add it to exclusion list)
22:02:56.32 +40:46:06.8 -- not an asteroid (will add it to exclusion list)
22:00:26.34 +35:56:03.5 -- not an asteroid (will add it to exclusion list)
21:51:26.79 +38:24:24.2 -- not an asteroid (will add it to exclusion list)
21:41:11.94 +41:00:50.9 -- not an asteroid (will add it to exclusion list)
21:50:25.25 +38:28:29.4 -- not an asteroid (will add it to exclusion list)
22:03:02.51 +36:29:37.6 -- not an asteroid (will add it to exclusion list)
21:46:04.46 +34:31:28.8 -- not an asteroid (will add it to exclusion list)
22:00:22.58 +36:02:18.8 -- not an asteroid (will add it to exclusion list)
21:56:03.61 +38:29:55.7 -- not an asteroid (will add it to exclusion list)
21:28:12.79 +36:49:25.2 -- not an asteroid (will add it to exclusion list)
21:55:53.68 +42:08:36.5 -- not an asteroid (will add it to exclusion list)
21:31:19.68 +39:08:30.9 -- not an asteroid (will add it to exclusion list)
21:51:41.99 +34:07:03.5 -- not an asteroid (will add it to exclusion list)
21:44:02.27 +38:24:38.7 -- not an asteroid (will add it to exclusion list)
21:43:24.81 +37:27:40.2 -- not an asteroid (will add it to exclusion list)
21:41:57.73 +41:24:19.5 -- not an asteroid (will add it to exclusion list)
21:42:33.81 +41:45:50.4 -- not an asteroid (will add it to exclusion list)
22:07:12.31 +41:10:46.1 -- not an asteroid (will add it to exclusion list)
21:29:22.39 +34:26:40.6 -- not an asteroid (will add it to exclusion list)
21:32:31.05 +37:13:03.8 -- not an asteroid (will add it to exclusion list)
22:09:10.52 +33:47:36.6 -- not an asteroid (will add it to exclusion list)
22:03:26.52 +35:25:29.3 -- not an asteroid (will add it to exclusion list)
21:41:45.31 +37:40:53.2 -- not an asteroid (will add it to exclusion list)
21:29:18.14 +33:38:40.5 -- not an asteroid (will add it to exclusion list)
22:08:01.57 +35:58:26.1 -- not an asteroid (will add it to exclusion list)
22:00:45.78 +42:12:40.6 -- not an asteroid (will add it to exclusion list)
21:44:03.17 +37:47:35.8 -- not an asteroid (will add it to exclusion list)
21:57:12.31 +36:23:41.2 -- not an asteroid (will add it to exclusion list)
21:49:03.73 +39:29:38.9 -- not an asteroid (will add it to exclusion list)
22:03:46.20 +38:55:41.6 -- not an asteroid (will add it to exclusion list)
21:53:48.08 +40:18:26.1 -- not an asteroid (will add it to exclusion list)
21:45:02.97 +36:40:08.0 -- not an asteroid (will add it to exclusion list)
22:08:21.44 +34:16:43.6 -- not an asteroid (will add it to exclusion list)
21:34:49.80 +42:03:15.4 -- not an asteroid (will add it to exclusion list)
21:47:46.78 +37:36:30.0 -- not an asteroid (will add it to exclusion list)
21:29:00.32 +38:59:30.2 -- not an asteroid (will add it to exclusion list)
21:35:25.71 +40:25:30.5 -- not an asteroid (will add it to exclusion list)
21:27:28.02 +39:54:38.6 -- not an asteroid (will add it to exclusion list)
21:53:31.10 +33:46:49.4 -- not an asteroid (will add it to exclusion list)
21:50:38.82 +39:20:18.3 -- not an asteroid (will add it to exclusion list)
21:46:35.91 +37:00:51.7 -- not an asteroid (will add it to exclusion list)
21:28:06.42 +33:41:27.0 -- not an asteroid (will add it to exclusion list)
22:07:48.92 +34:48:03.5 -- not an asteroid (will add it to exclusion list)
22:05:32.49 +38:58:33.0 -- not an asteroid (will add it to exclusion list)
21:51:31.60 +37:29:39.0 -- not an asteroid (will add it to exclusion list)
21:50:30.82 +36:49:51.1 -- not an asteroid (will add it to exclusion list)
22:00:16.07 +41:05:52.9 -- not an asteroid (will add it to exclusion list)
21:29:46.34 +35:53:26.3 -- not an asteroid (will add it to exclusion list)
21:57:31.30 +38:48:28.0 -- not an asteroid (will add it to exclusion list)
21:44:09.01 +35:27:53.6 -- not an asteroid (will add it to exclusion list)
21:43:02.34 +34:00:48.1 -- not an asteroid (will add it to exclusion list)
21:32:45.10 +38:02:03.6 -- not an asteroid (will add it to exclusion list)
21:51:29.81 +37:52:05.2 -- not an asteroid (will add it to exclusion list)
21:42:51.49 +37:11:24.5 -- not an asteroid (will add it to exclusion list)
22:02:54.23 +40:52:40.1 -- not an asteroid (will add it to exclusion list)
21:42:39.00 +37:00:24.2 -- not an asteroid (will add it to exclusion list)
22:08:57.22 +36:50:52.7 -- not an asteroid (will add it to exclusion list)
21:40:15.60 +37:50:20.1 -- not an asteroid (will add it to exclusion list)
22:07:52.46 +41:59:46.9 -- not an asteroid (will add it to exclusion list)
22:10:57.04 +37:02:43.5 -- not an asteroid (will add it to exclusion list)
22:06:24.16 +38:41:47.2 -- not an asteroid (will add it to exclusion list)
21:26:26.98 +37:43:49.9 -- not an asteroid (will add it to exclusion list)
21:40:39.67 +36:27:52.9 -- not an asteroid (will add it to exclusion list)
21:55:19.69 +36:41:47.8 -- not an asteroid (will add it to exclusion list)
21:26:40.74 +39:52:49.0 -- not an asteroid (will add it to exclusion list)
21:43:23.84 +33:45:14.5 -- not an asteroid (will add it to exclusion list)
21:43:17.63 +38:29:48.8 -- not an asteroid (will add it to exclusion list)
22:03:38.17 +36:16:08.0 -- not an asteroid (will add it to exclusion list)
21:58:28.78 +40:10:17.0 -- not an asteroid (will add it to exclusion list)
21:57:14.45 +42:01:03.9 -- not an asteroid (will add it to exclusion list)
21:33:10.28 +41:39:56.3 -- not an asteroid (will add it to exclusion list)
21:28:22.15 +41:32:00.3 -- not an asteroid (will add it to exclusion list)
21:29:16.83 +34:43:07.0 -- not an asteroid (will add it to exclusion list)
22:04:23.77 +39:34:05.5 -- not an asteroid (will add it to exclusion list)
22:05:37.45 +38:57:41.0 -- not an asteroid (will add it to exclusion list)
21:54:38.60 +36:53:53.5 -- not an asteroid (will add it to exclusion list)
21:30:29.91 +39:49:30.6 -- not an asteroid (will add it to exclusion list)
21:48:12.58 +41:41:12.5 -- not an asteroid (will add it to exclusion list)
21:30:08.27 +37:30:28.0 -- not an asteroid (will add it to exclusion list)
21:45:30.14 +42:12:25.2 -- not an asteroid (will add it to exclusion list)
22:03:06.42 +40:42:37.9 -- not an asteroid (will add it to exclusion list)
21:44:13.05 +38:35:36.7 -- not an asteroid (will add it to exclusion list)
21:58:00.76 +37:39:30.9 -- not an asteroid (will add it to exclusion list)
21:28:31.47 +41:22:58.2 -- not an asteroid (will add it to exclusion list)
21:31:31.11 +41:31:49.7 -- not an asteroid (will add it to exclusion list)
22:01:22.48 +40:55:08.5 -- not an asteroid (will add it to exclusion list)
21:40:43.84 +37:22:59.4 -- not an asteroid (will add it to exclusion list)
21:40:26.40 +39:27:29.0 -- not an asteroid (will add it to exclusion list)
21:33:11.14 +39:46:10.4 -- not an asteroid (will add it to exclusion list)
22:02:11.40 +35:32:41.6 -- not an asteroid (will add it to exclusion list)
21:49:22.29 +41:57:46.4 -- not an asteroid (will add it to exclusion list)
21:57:39.33 +41:47:18.3 -- not an asteroid (will add it to exclusion list)
21:50:25.17 +35:00:16.6 -- not an asteroid (will add it to exclusion list)
21:30:28.13 +38:52:35.3 -- not an asteroid (will add it to exclusion list)
21:35:35.36 +35:59:26.5 -- not an asteroid (will add it to exclusion list)
21:34:37.63 +34:15:56.3 -- not an asteroid (will add it to exclusion list)
22:10:32.03 +41:45:05.9 -- not an asteroid (will add it to exclusion list)
22:11:02.23 +38:11:05.6 -- not an asteroid (will add it to exclusion list)
22:12:04.92 +39:17:50.0 -- not an asteroid (will add it to exclusion list)
21:40:56.14 +41:13:20.7 -- not an asteroid (will add it to exclusion list)
22:07:02.72 +41:57:30.8 -- not an asteroid (will add it to exclusion list)
21:44:09.61 +37:55:02.7 -- not an asteroid (will add it to exclusion list)
21:33:22.18 +38:02:28.7 -- not an asteroid (will add it to exclusion list)
22:05:39.89 +34:53:38.5 -- not an asteroid (will add it to exclusion list)
21:33:13.81 +37:12:44.0 -- not an asteroid (will add it to exclusion list)
21:59:20.91 +36:56:49.2 -- not an asteroid (will add it to exclusion list)
22:06:30.62 +34:18:24.6 -- not an asteroid (will add it to exclusion list)
21:59:59.23 +36:08:33.3 -- not an asteroid (will add it to exclusion list)
21:37:46.88 +36:44:34.4 -- not an asteroid (will add it to exclusion list)
21:28:09.30 +41:14:37.1 -- not an asteroid (will add it to exclusion list)
21:32:51.76 +35:15:25.9 -- not an asteroid (will add it to exclusion list)
21:56:52.31 +39:21:22.0 -- not an asteroid (will add it to exclusion list)
21:27:20.05 +35:46:48.2 -- not an asteroid (will add it to exclusion list)
21:28:11.99 +34:45:25.7 -- not an asteroid (will add it to exclusion list)
21:54:25.08 +39:39:28.0 -- not an asteroid (will add it to exclusion list)
21:30:32.04 +35:46:44.4 -- not an asteroid (will add it to exclusion list)
21:46:48.64 +36:53:20.3 -- not an asteroid (will add it to exclusion list)
21:38:15.46 +38:02:08.4 -- not an asteroid (will add it to exclusion list)
21:36:49.67 +39:45:20.6 -- not an asteroid (will add it to exclusion list)
22:06:56.78 +36:48:40.3 -- not an asteroid (will add it to exclusion list)
22:00:17.84 +38:06:34.9 -- not an asteroid (will add it to exclusion list)
21:59:06.43 +34:00:17.5 -- not an asteroid (will add it to exclusion list)
22:01:18.69 +41:30:27.6 -- not an asteroid (will add it to exclusion list)
21:34:29.38 +39:23:38.8 -- not an asteroid (will add it to exclusion list)
22:01:14.44 +38:33:47.4 -- not an asteroid (will add it to exclusion list)
21:31:14.97 +38:46:29.7 -- not an asteroid (will add it to exclusion list)
22:09:13.59 +39:15:46.5 -- not an asteroid (will add it to exclusion list)
21:44:42.94 +35:29:07.5 -- not an asteroid (will add it to exclusion list)
22:02:13.94 +41:47:07.6 -- not an asteroid (will add it to exclusion list)
21:43:06.26 +37:12:23.6 -- not an asteroid (will add it to exclusion list)
21:40:41.05 +36:19:20.5 -- not an asteroid (will add it to exclusion list)
22:02:42.11 +37:08:59.4 -- not an asteroid (will add it to exclusion list)
22:02:14.92 +34:37:08.3 -- not an asteroid (will add it to exclusion list)
22:02:42.57 +41:44:09.7 -- not an asteroid (will add it to exclusion list)
22:00:24.33 +35:58:53.7 -- not an asteroid (will add it to exclusion list)
22:03:19.33 +33:44:47.9 -- not an asteroid (will add it to exclusion list)
22:10:02.92 +36:44:11.9 -- not an asteroid (will add it to exclusion list)
21:49:08.07 +35:40:21.4 -- not an asteroid (will add it to exclusion list)
22:06:31.92 +34:33:33.0 -- not an asteroid (will add it to exclusion list)
21:54:12.72 +35:10:05.1 -- not an asteroid (will add it to exclusion list)
21:40:47.62 +37:32:56.2 -- not an asteroid (will add it to exclusion list)
22:09:46.32 +41:39:59.1 -- not an asteroid (will add it to exclusion list)
21:47:33.77 +37:22:55.8 -- not an asteroid (will add it to exclusion list)
21:33:58.57 +36:17:17.8 -- not an asteroid (will add it to exclusion list)
22:04:59.77 +39:57:17.5 -- not an asteroid (will add it to exclusion list)
21:48:15.82 +35:31:04.0 -- not an asteroid (will add it to exclusion list)
22:02:04.72 +37:45:26.3 -- not an asteroid (will add it to exclusion list)
21:54:39.47 +39:49:48.7 -- not an asteroid (will add it to exclusion list)
22:11:31.18 +40:27:17.9 -- not an asteroid (will add it to exclusion list)
22:05:42.70 +35:53:01.6 -- not an asteroid (will add it to exclusion list)
21:48:57.95 +37:42:52.3 -- not an asteroid (will add it to exclusion list)
21:58:42.71 +38:46:43.2 -- not an asteroid (will add it to exclusion list)
22:10:20.20 +38:44:20.8 -- not an asteroid (will add it to exclusion list)
21:58:43.33 +42:11:57.9 -- not an asteroid (will add it to exclusion list)
21:49:41.31 +37:43:29.6 -- not an asteroid (will add it to exclusion list)
21:51:57.64 +37:11:55.0 -- not an asteroid (will add it to exclusion list)
22:06:28.76 +39:03:18.4 -- not an asteroid (will add it to exclusion list)
22:00:37.00 +35:01:34.4 -- not an asteroid (will add it to exclusion list)
21:59:40.08 +41:01:41.0 -- not an asteroid (will add it to exclusion list)
22:00:24.47 +39:57:06.7 -- not an asteroid (will add it to exclusion list)
22:07:43.41 +37:37:06.0 -- not an asteroid (will add it to exclusion list)
22:01:04.09 +41:04:55.5 -- not an asteroid (will add it to exclusion list)
22:11:43.30 +42:07:49.5 -- not an asteroid (will add it to exclusion list)
21:36:14.22 +40:15:40.1 -- not an asteroid (will add it to exclusion list)
21:33:15.00 +33:54:30.0 -- not an asteroid (will add it to exclusion list)
21:56:29.42 +36:52:34.4 -- not an asteroid (will add it to exclusion list)
21:59:28.83 +37:59:48.3 -- not an asteroid (will add it to exclusion list)
21:35:57.86 +41:51:55.7 -- not an asteroid (will add it to exclusion list)
22:09:11.66 +36:46:05.4 -- not an asteroid (will add it to exclusion list)
21:41:04.38 +37:16:08.3 -- not an asteroid (will add it to exclusion list)
21:58:52.18 +37:02:33.4 -- not an asteroid (will add it to exclusion list)
22:09:33.65 +41:54:58.8 -- not an asteroid (will add it to exclusion list)
21:51:03.60 +36:58:53.3 -- not an asteroid (will add it to exclusion list)
22:02:20.04 +34:02:55.5 -- not an asteroid (will add it to exclusion list)
21:47:12.13 +36:46:39.3 -- not an asteroid (will add it to exclusion list)
21:55:27.21 +41:39:30.1 -- not an asteroid (will add it to exclusion list)
21:46:37.68 +36:31:34.8 -- not an asteroid (will add it to exclusion list)
22:01:20.19 +41:45:32.7 -- not an asteroid (will add it to exclusion list)
21:57:35.09 +40:21:27.2 -- not an asteroid (will add it to exclusion list)
21:48:08.00 +39:26:18.8 -- not an asteroid (will add it to exclusion list)
21:59:05.04 +35:36:42.6 -- not an asteroid (will add it to exclusion list)
21:50:41.80 +36:02:33.6 -- not an asteroid (will add it to exclusion list)
22:04:54.69 +35:49:32.1 -- not an asteroid (will add it to exclusion list)
22:09:59.93 +38:20:08.0 -- not an asteroid (will add it to exclusion list)
21:27:56.81 +35:27:16.8 -- not an asteroid (will add it to exclusion list)
21:39:40.95 +34:24:59.2 -- not an asteroid (will add it to exclusion list)
21:27:07.34 +35:14:58.4 -- not an asteroid (will add it to exclusion list)
21:38:09.32 +36:54:28.0 -- not an asteroid (will add it to exclusion list)
21:49:15.19 +35:18:21.5 -- not an asteroid (will add it to exclusion list)
22:00:15.80 +35:08:28.9 -- not an asteroid (will add it to exclusion list)
21:32:14.37 +37:49:10.6 -- not an asteroid (will add it to exclusion list)
22:02:05.91 +41:42:42.0 -- not an asteroid (will add it to exclusion list)
21:57:10.60 +42:10:41.6 -- not an asteroid (will add it to exclusion list)
22:06:23.77 +41:39:59.2 -- not an asteroid (will add it to exclusion list)
21:26:46.13 +37:00:02.7 -- not an asteroid (will add it to exclusion list)
21:56:00.58 +37:10:57.1 -- not an asteroid (will add it to exclusion list)
22:04:05.48 +41:13:37.3 -- not an asteroid (will add it to exclusion list)
21:57:11.29 +40:23:42.7 -- not an asteroid (will add it to exclusion list)
22:05:58.50 +41:55:51.3 -- not an asteroid (will add it to exclusion list)
21:50:34.42 +37:11:03.5 -- not an asteroid (will add it to exclusion list)
21:59:31.05 +42:08:24.3 -- not an asteroid (will add it to exclusion list)
22:10:36.56 +39:03:13.4 -- not an asteroid (will add it to exclusion list)
21:37:13.77 +40:19:25.1 -- not an asteroid (will add it to exclusion list)
22:06:38.72 +41:43:51.1 -- not an asteroid (will add it to exclusion list)
21:39:53.74 +37:58:53.1 -- not an asteroid (will add it to exclusion list)
21:48:46.74 +35:26:20.4 -- not an asteroid (will add it to exclusion list)
21:46:54.04 +39:15:19.9 -- not an asteroid (will add it to exclusion list)
21:56:34.64 +37:00:25.7 -- not an asteroid (will add it to exclusion list)
21:59:09.95 +36:16:48.9 -- not an asteroid (will add it to exclusion list)
21:39:06.45 +37:40:27.9 -- not an asteroid (will add it to exclusion list)
21:59:27.03 +41:38:40.6 -- not an asteroid (will add it to exclusion list)
21:34:22.92 +34:51:23.4 -- not an asteroid (will add it to exclusion list)
22:05:37.91 +35:36:47.0 -- not an asteroid (will add it to exclusion list)
22:01:12.35 +35:17:06.2 -- not an asteroid (will add it to exclusion list)
21:47:32.63 +41:45:11.6 -- not an asteroid (will add it to exclusion list)
22:06:02.05 +40:00:16.4 -- not an asteroid (will add it to exclusion list)
21:48:47.80 +38:52:57.8 -- not an asteroid (will add it to exclusion list)
21:47:31.33 +37:36:09.6 -- not an asteroid (will add it to exclusion list)
21:35:24.09 +36:47:16.4 -- not an asteroid (will add it to exclusion list)
21:41:32.72 +36:23:15.4 -- not an asteroid (will add it to exclusion list)
21:50:58.78 +36:44:37.4 -- not an asteroid (will add it to exclusion list)
22:00:17.81 +40:36:29.5 -- not an asteroid (will add it to exclusion list)
21:46:12.49 +39:34:00.4 -- not an asteroid (will add it to exclusion list)
21:53:41.44 +40:47:14.5 -- not an asteroid (will add it to exclusion list)
21:50:08.02 +34:33:28.4 -- not an asteroid (will add it to exclusion list)
22:06:37.68 +41:44:03.3 -- not an asteroid (will add it to exclusion list)
21:28:43.59 +35:11:02.7 -- not an asteroid (will add it to exclusion list)
21:27:00.76 +33:45:02.8 -- not an asteroid (will add it to exclusion list)
21:28:43.73 +35:42:02.4 -- not an asteroid (will add it to exclusion list)
22:06:09.41 +39:56:12.0 -- not an asteroid (will add it to exclusion list)
21:44:51.80 +36:12:12.5 -- not an asteroid (will add it to exclusion list)
21:54:32.82 +35:25:31.7 -- not an asteroid (will add it to exclusion list)
22:00:56.16 +36:53:36.2 -- not an asteroid (will add it to exclusion list)
21:47:51.58 +40:21:48.5 -- not an asteroid (will add it to exclusion list)
21:40:34.69 +33:42:27.1 -- not an asteroid (will add it to exclusion list)
21:45:18.29 +37:39:34.8 -- not an asteroid (will add it to exclusion list)
22:02:17.99 +35:48:05.0 -- not an asteroid (will add it to exclusion list)
22:04:46.29 +42:08:02.1 -- not an asteroid (will add it to exclusion list)
21:32:06.91 +39:41:52.6 -- not an asteroid (will add it to exclusion list)
21:36:58.26 +37:51:36.1 -- not an asteroid (will add it to exclusion list)
22:02:38.99 +37:13:44.3 -- not an asteroid (will add it to exclusion list)
21:41:05.04 +34:50:47.1 -- not an asteroid (will add it to exclusion list)
21:29:38.98 +36:14:25.4 -- not an asteroid (will add it to exclusion list)
21:55:36.33 +35:51:32.4 -- not an asteroid (will add it to exclusion list)
21:54:51.04 +40:07:59.2 -- not an asteroid (will add it to exclusion list)
22:01:06.63 +42:14:36.5 -- not an asteroid (will add it to exclusion list)
21:49:28.23 +38:12:27.0 -- not an asteroid (will add it to exclusion list)
22:04:39.48 +41:55:44.1 -- not an asteroid (will add it to exclusion list)
21:50:44.44 +36:27:35.4 -- not an asteroid (will add it to exclusion list)
21:59:42.10 +41:00:46.6 -- not an asteroid (will add it to exclusion list)
21:36:16.89 +35:02:27.0 -- not an asteroid (will add it to exclusion list)
22:08:10.70 +39:02:02.5 -- not an asteroid (will add it to exclusion list)
21:31:29.68 +33:55:39.8 -- not an asteroid (will add it to exclusion list)
22:04:12.58 +40:40:22.1 -- not an asteroid (will add it to exclusion list)
21:33:29.30 +37:59:54.7 -- not an asteroid (will add it to exclusion list)
22:06:29.11 +39:32:46.8 -- not an asteroid (will add it to exclusion list)
22:00:45.71 +42:12:57.5 -- not an asteroid (will add it to exclusion list)
22:04:43.21 +42:01:06.8 -- not an asteroid (will add it to exclusion list)
22:08:49.92 +40:21:08.2 -- not an asteroid (will add it to exclusion list)
21:32:35.91 +35:36:09.9 -- not an asteroid (will add it to exclusion list)
22:03:59.79 +41:38:51.3 -- not an asteroid (will add it to exclusion list)
22:10:43.52 +41:09:26.3 -- not an asteroid (will add it to exclusion list)
21:52:14.12 +37:49:46.3 -- not an asteroid (will add it to exclusion list)
21:53:37.65 +42:15:49.5 -- not an asteroid (will add it to exclusion list)
22:06:12.37 +39:36:03.7 -- not an asteroid (will add it to exclusion list)
22:04:30.32 +41:26:44.7 -- not an asteroid (will add it to exclusion list)
21:58:23.87 +37:48:10.5 -- not an asteroid (will add it to exclusion list)
22:00:09.65 +33:45:56.1 -- not an asteroid (will add it to exclusion list)
21:35:34.13 +34:35:52.2 -- not an asteroid (will add it to exclusion list)
21:30:30.66 +33:57:26.0 -- not an asteroid (will add it to exclusion list)
21:33:29.11 +33:39:19.5 -- not an asteroid (will add it to exclusion list)
21:52:15.43 +41:18:16.1 -- not an asteroid (will add it to exclusion list)
21:50:17.59 +42:04:56.5 -- not an asteroid (will add it to exclusion list)
21:52:31.29 +41:07:39.3 -- not an asteroid (will add it to exclusion list)
21:56:04.82 +37:14:36.4 -- not an asteroid (will add it to exclusion list)
21:49:25.96 +38:25:18.2 -- not an asteroid (will add it to exclusion list)
21:39:26.02 +34:58:46.9 -- not an asteroid (will add it to exclusion list)
21:58:33.10 +38:59:49.3 -- not an asteroid (will add it to exclusion list)
21:26:55.25 +38:03:55.3 -- not an asteroid (will add it to exclusion list)
22:11:45.13 +41:45:55.6 -- not an asteroid (will add it to exclusion list)
22:08:58.89 +42:02:06.8 -- not an asteroid (will add it to exclusion list)
22:07:35.18 +41:27:44.3 -- not an asteroid (will add it to exclusion list)
22:05:27.15 +41:32:30.4 -- not an asteroid (will add it to exclusion list)
21:56:45.81 +40:47:17.0 -- not an asteroid (will add it to exclusion list)
21:27:12.50 +33:51:25.4 -- not an asteroid (will add it to exclusion list)
21:35:21.65 +41:16:19.3 -- not an asteroid (will add it to exclusion list)
22:01:09.64 +39:37:09.0 -- not an asteroid (will add it to exclusion list)
21:40:12.93 +34:16:54.1 -- not an asteroid (will add it to exclusion list)
21:34:45.74 +38:35:14.3 -- not an asteroid (will add it to exclusion list)
22:03:08.35 +41:49:49.0 -- not an asteroid (will add it to exclusion list)
21:40:44.27 +35:27:41.7 -- not an asteroid (will add it to exclusion list)
22:10:20.81 +41:33:09.1 -- not an asteroid (will add it to exclusion list)
21:36:24.02 +37:34:32.2 -- not an asteroid (will add it to exclusion list)
21:43:05.91 +37:32:44.3 -- not an asteroid (will add it to exclusion list)
21:52:59.24 +34:14:49.0 -- not an asteroid (will add it to exclusion list)
21:41:44.91 +34:02:40.1 -- not an asteroid (will add it to exclusion list)
22:07:10.96 +38:37:34.4 -- not an asteroid (will add it to exclusion list)
22:05:48.96 +40:22:58.1 -- not an asteroid (will add it to exclusion list)
22:10:14.91 +41:02:14.0 -- not an asteroid (will add it to exclusion list)
22:09:51.75 +41:55:24.7 -- not an asteroid (will add it to exclusion list)
21:51:40.11 +38:49:49.1 -- not an asteroid (will add it to exclusion list)
22:00:13.75 +41:45:18.1 -- not an asteroid (will add it to exclusion list)
22:07:23.06 +41:08:43.2 -- not an asteroid (will add it to exclusion list)
21:57:53.26 +36:58:24.0 -- not an asteroid (will add it to exclusion list)
22:00:13.35 +34:58:25.7 -- not an asteroid (will add it to exclusion list)
22:08:34.63 +37:33:22.7 -- not an asteroid (will add it to exclusion list)
22:00:06.38 +39:09:22.8 -- not an asteroid (will add it to exclusion list)
21:37:32.90 +34:45:17.1 -- not an asteroid (will add it to exclusion list)
21:28:20.93 +36:09:00.3 -- not an asteroid (will add it to exclusion list)
21:53:14.97 +36:41:36.6 -- not an asteroid (will add it to exclusion list)
21:53:00.65 +35:46:13.8 -- not an asteroid (will add it to exclusion list)
21:30:41.28 +35:07:19.3 -- not an asteroid (will add it to exclusion list)
22:01:24.44 +41:55:51.4 -- not an asteroid (will add it to exclusion list)
21:30:30.84 +40:52:58.5 -- not an asteroid (will add it to exclusion list)
21:44:43.69 +35:06:39.2 -- not an asteroid (will add it to exclusion list)
22:11:07.15 +41:20:25.4 -- not an asteroid (will add it to exclusion list)
21:57:39.47 +41:25:20.3 -- not an asteroid (will add it to exclusion list)
21:37:29.63 +35:54:14.5 -- not an asteroid (will add it to exclusion list)
21:50:22.68 +40:29:52.1 -- not an asteroid (will add it to exclusion list)
22:12:24.03 +40:35:38.7 -- not an asteroid (will add it to exclusion list)
21:35:41.21 +35:13:20.9 -- not an asteroid (will add it to exclusion list)
21:36:41.98 +36:15:49.7 -- not an asteroid (will add it to exclusion list)
21:36:58.91 +34:31:59.2 -- not an asteroid (will add it to exclusion list)
21:39:50.75 +37:38:28.6 -- not an asteroid (will add it to exclusion list)
21:30:39.34 +38:36:14.0 -- not an asteroid (will add it to exclusion list)
22:03:04.95 +35:09:33.5 -- not an asteroid (will add it to exclusion list)
21:31:32.90 +33:56:49.8 -- not an asteroid (will add it to exclusion list)
22:07:22.71 +40:35:19.9 -- not an asteroid (will add it to exclusion list)
22:04:34.65 +36:25:09.6 -- not an asteroid (will add it to exclusion list)
21:44:23.69 +38:52:48.1 -- not an asteroid (will add it to exclusion list)
21:51:39.19 +36:55:28.8 -- not an asteroid (will add it to exclusion list)
22:02:22.69 +41:34:47.5 -- not an asteroid (will add it to exclusion list)
21:52:45.65 +42:15:35.3 -- not an asteroid (will add it to exclusion list)
21:31:39.39 +36:46:29.2 -- not an asteroid (will add it to exclusion list)
21:37:58.77 +36:42:07.1 -- not an asteroid (will add it to exclusion list)
22:09:55.37 +40:48:12.0 -- not an asteroid (will add it to exclusion list)
21:52:44.60 +34:42:49.6 -- not an asteroid (will add it to exclusion list)
22:05:09.75 +37:59:07.1 -- not an asteroid (will add it to exclusion list)
21:45:12.02 +40:36:35.5 -- not an asteroid (will add it to exclusion list)
21:56:15.10 +41:22:11.4 -- not an asteroid (will add it to exclusion list)
21:53:39.07 +34:51:16.0 -- not an asteroid (will add it to exclusion list)
21:50:55.25 +34:16:15.5 -- not an asteroid (will add it to exclusion list)
21:51:03.23 +33:59:27.0 -- not an asteroid (will add it to exclusion list)
22:08:43.68 +41:30:45.0 -- not an asteroid (will add it to exclusion list)
22:11:12.81 +41:39:57.6 -- not an asteroid (will add it to exclusion list)
22:11:35.58 +41:59:08.7 -- not an asteroid (will add it to exclusion list)
21:51:22.88 +33:49:09.9 -- not an asteroid (will add it to exclusion list)
21:40:21.22 +39:47:14.7 -- not an asteroid (will add it to exclusion list)
22:11:52.00 +42:03:53.3 -- not an asteroid (will add it to exclusion list)
21:51:12.70 +35:28:48.9 -- not an asteroid (will add it to exclusion list)
21:27:06.61 +33:44:10.1 -- not an asteroid (will add it to exclusion list)
22:05:27.65 +42:00:52.5 -- not an asteroid (will add it to exclusion list)
22:02:10.53 +42:07:01.9 -- not an asteroid (will add it to exclusion list)
21:29:16.00 +34:53:37.5 -- not an asteroid (will add it to exclusion list)
22:02:41.97 +41:43:44.0 -- not an asteroid (will add it to exclusion list)
21:53:20.58 +39:06:18.6 -- not an asteroid (will add it to exclusion list)
21:26:51.68 +34:03:09.6 -- not an asteroid (will add it to exclusion list)
21:46:38.91 +34:22:59.8 -- not an asteroid (will add it to exclusion list)
21:59:56.19 +38:33:11.5 -- not an asteroid (will add it to exclusion list)
21:30:22.42 +38:20:38.9 -- not an asteroid (will add it to exclusion list)
22:08:02.15 +37:33:32.4 -- not an asteroid (will add it to exclusion list)
21:33:52.98 +36:12:28.2 -- not an asteroid (will add it to exclusion list)
21:40:55.51 +35:54:46.3 -- not an asteroid (will add it to exclusion list)
21:58:32.72 +37:55:01.1 -- not an asteroid (will add it to exclusion list)
21:50:35.57 +37:36:20.8 -- not an asteroid (will add it to exclusion list)
21:29:24.07 +33:58:30.2 -- not an asteroid (will add it to exclusion list)
21:28:04.99 +35:56:21.6 -- not an asteroid (will add it to exclusion list)
21:31:40.91 +33:48:11.1 -- not an asteroid (will add it to exclusion list)
21:54:19.06 +34:21:38.0 -- not an asteroid (will add it to exclusion list)
22:10:15.85 +41:34:00.4 -- not an asteroid (will add it to exclusion list)
21:26:53.85 +33:43:13.3 -- not an asteroid (will add it to exclusion list)
21:33:23.27 +35:48:05.1 -- not an asteroid (will add it to exclusion list)
21:32:38.78 +34:43:55.9 -- not an asteroid (will add it to exclusion list)
21:59:50.53 +41:52:08.1 -- not an asteroid (will add it to exclusion list)
21:58:43.93 +39:44:49.6 -- not an asteroid (will add it to exclusion list)
21:34:30.55 +33:45:42.3 -- not an asteroid (will add it to exclusion list)
21:58:36.26 +41:09:23.1 -- not an asteroid (will add it to exclusion list)
21:50:53.08 +37:38:05.3 -- not an asteroid (will add it to exclusion list)
21:52:19.93 +39:44:46.8 -- not an asteroid (will add it to exclusion list)
22:04:44.36 +37:33:00.6 -- not an asteroid (will add it to exclusion list)
22:07:31.14 +39:46:41.6 -- not an asteroid (will add it to exclusion list)
22:03:12.98 +39:06:03.2 -- not an asteroid (will add it to exclusion list)
21:31:57.30 +36:19:02.3 -- not an asteroid (will add it to exclusion list)
21:51:11.92 +37:00:41.8 -- not an asteroid (will add it to exclusion list)
21:42:31.31 +35:51:14.4 -- not an asteroid (will add it to exclusion list)
21:39:23.59 +37:37:07.9 -- not an asteroid (will add it to exclusion list)
21:28:08.29 +36:20:37.2 -- not an asteroid (will add it to exclusion list)
21:37:02.85 +36:17:37.9 -- not an asteroid (will add it to exclusion list)
21:29:00.99 +33:49:52.9 -- not an asteroid (will add it to exclusion list)
21:54:45.91 +38:18:19.5 -- not an asteroid (will add it to exclusion list)
21:50:56.50 +33:55:09.6 -- not an asteroid (will add it to exclusion list)
21:58:49.54 +40:28:43.1 -- not an asteroid (will add it to exclusion list)
22:08:28.16 +41:17:32.5 -- not an asteroid (will add it to exclusion list)
21:55:07.10 +38:37:59.5 -- not an asteroid (will add it to exclusion list)
21:28:55.84 +39:02:12.2 -- not an asteroid (will add it to exclusion list)
21:30:33.16 +34:04:09.8 -- not an asteroid (will add it to exclusion list)
21:47:46.25 +35:56:49.8 -- not an asteroid (will add it to exclusion list)
21:43:50.45 +37:03:22.9 -- not an asteroid (will add it to exclusion list)
21:50:07.74 +42:10:51.9 -- not an asteroid (will add it to exclusion list)
21:31:26.89 +33:46:05.5 -- not an asteroid (will add it to exclusion list)
21:49:09.64 +42:12:56.5 -- not an asteroid (will add it to exclusion list)
21:56:26.04 +37:57:07.1 -- not an asteroid (will add it to exclusion list)
22:12:02.15 +41:01:53.3 -- not an asteroid (will add it to exclusion list)
22:03:19.70 +38:40:39.2 -- not an asteroid (will add it to exclusion list)
21:47:53.10 +34:00:34.1 -- not an asteroid (will add it to exclusion list)
21:49:59.42 +34:39:56.9 -- not an asteroid (will add it to exclusion list)
22:08:12.38 +39:44:12.0 -- not an asteroid (will add it to exclusion list)
21:46:56.92 +41:43:39.2 -- not an asteroid (will add it to exclusion list)
21:36:08.48 +35:55:06.2 -- not an asteroid (will add it to exclusion list)
22:06:05.56 +41:38:13.1 -- not an asteroid (will add it to exclusion list)
21:45:54.78 +36:04:45.0 -- not an asteroid (will add it to exclusion list)
21:43:24.22 +39:02:44.7 -- not an asteroid (will add it to exclusion list)
21:54:13.84 +42:03:14.7 -- not an asteroid (will add it to exclusion list)
22:03:45.58 +37:16:45.0 -- not an asteroid (will add it to exclusion list)
21:58:01.47 +38:57:27.0 -- not an asteroid (will add it to exclusion list)
21:49:19.26 +36:58:39.0 -- not an asteroid (will add it to exclusion list)
21:52:57.14 +41:56:24.0 -- not an asteroid (will add it to exclusion list)
21:59:54.31 +34:16:50.9 -- not an asteroid (will add it to exclusion list)
21:55:11.88 +36:28:56.0 -- not an asteroid (will add it to exclusion list)
22:01:30.08 +41:04:28.8 -- not an asteroid (will add it to exclusion list)
22:00:40.88 +34:40:45.0 -- not an asteroid (will add it to exclusion list)
21:28:15.82 +34:43:42.3 -- not an asteroid (will add it to exclusion list)
21:33:16.16 +41:46:48.3 -- not an asteroid (will add it to exclusion list)
22:00:20.90 +41:35:27.5 -- not an asteroid (will add it to exclusion list)
22:08:56.95 +41:29:27.8 -- not an asteroid (will add it to exclusion list)
21:58:48.24 +40:45:27.6 -- not an asteroid (will add it to exclusion list)
21:38:03.92 +38:03:50.8 -- not an asteroid (will add it to exclusion list)
21:48:31.78 +39:16:35.8 -- not an asteroid (will add it to exclusion list)
21:55:20.84 +34:39:46.5 -- not an asteroid (will add it to exclusion list)
21:42:21.52 +36:16:15.6 -- not an asteroid (will add it to exclusion list)
22:02:43.72 +35:30:17.9 -- not an asteroid (will add it to exclusion list)
21:34:31.83 +40:00:34.5 -- not an asteroid (will add it to exclusion list)
21:54:17.40 +36:52:10.6 -- not an asteroid (will add it to exclusion list)
21:37:03.51 +37:31:36.8 -- not an asteroid (will add it to exclusion list)
22:04:39.71 +37:04:27.3 -- not an asteroid (will add it to exclusion list)
21:57:38.67 +36:43:41.1 -- not an asteroid (will add it to exclusion list)
21:59:07.04 +37:35:41.8 -- not an asteroid (will add it to exclusion list)
21:29:05.04 +40:36:55.7 -- not an asteroid (will add it to exclusion list)
21:33:40.02 +33:37:46.0 -- not an asteroid (will add it to exclusion list)
21:33:43.05 +37:03:45.6 -- not an asteroid (will add it to exclusion list)
22:08:55.68 +38:16:52.9 -- not an asteroid (will add it to exclusion list)
21:53:51.27 +33:51:00.5 -- not an asteroid (will add it to exclusion list)
21:27:30.62 +35:18:41.9 -- not an asteroid (will add it to exclusion list)
21:51:39.59 +40:18:36.0 -- not an asteroid (will add it to exclusion list)
22:02:49.10 +35:57:04.6 -- not an asteroid (will add it to exclusion list)
21:37:17.02 +36:54:05.4 -- not an asteroid (will add it to exclusion list)
21:49:30.28 +38:28:52.1 -- not an asteroid (will add it to exclusion list)
21:28:43.48 +36:04:03.7 -- not an asteroid (will add it to exclusion list)
22:00:10.43 +38:33:13.9 -- not an asteroid (will add it to exclusion list)
22:11:52.66 +40:52:48.1 -- not an asteroid (will add it to exclusion list)
21:43:28.90 +37:46:48.1 -- not an asteroid (will add it to exclusion list)
21:34:28.42 +40:12:23.8 -- not an asteroid (will add it to exclusion list)
22:11:50.18 +39:03:26.3 -- not an asteroid (will add it to exclusion list)
22:03:00.73 +38:51:52.9 -- not an asteroid (will add it to exclusion list)
21:57:52.96 +34:06:45.3 -- not an asteroid (will add it to exclusion list)
21:49:13.72 +35:11:21.8 -- not an asteroid (will add it to exclusion list)
22:02:05.34 +37:22:23.9 -- not an asteroid (will add it to exclusion list)
21:57:21.27 +37:30:14.8 -- not an asteroid (will add it to exclusion list)
21:42:25.14 +35:54:12.6 -- not an asteroid (will add it to exclusion list)
21:48:39.22 +37:49:35.3 -- not an asteroid (will add it to exclusion list)
21:44:01.36 +38:56:13.3 -- not an asteroid (will add it to exclusion list)
21:34:10.50 +35:44:49.6 -- not an asteroid (will add it to exclusion list)
22:01:39.44 +34:45:27.5 -- not an asteroid (will add it to exclusion list)
22:00:37.79 +41:43:04.1 -- not an asteroid (will add it to exclusion list)
21:54:53.71 +41:04:43.2 -- not an asteroid (will add it to exclusion list)
21:29:44.17 +35:02:48.4 -- not an asteroid (will add it to exclusion list)
21:59:17.07 +35:39:25.5 -- not an asteroid (will add it to exclusion list)
21:41:58.03 +35:21:26.8 -- not an asteroid (will add it to exclusion list)
22:04:41.21 +40:20:51.2 -- not an asteroid (will add it to exclusion list)
22:00:13.59 +38:25:18.0 -- not an asteroid (will add it to exclusion list)
21:46:22.62 +36:17:37.7 -- not an asteroid (will add it to exclusion list)
21:36:08.38 +34:28:55.9 -- not an asteroid (will add it to exclusion list)
21:58:26.35 +42:12:16.4 -- not an asteroid (will add it to exclusion list)
21:35:23.86 +34:51:32.9 -- not an asteroid (will add it to exclusion list)
21:31:17.69 +33:40:29.1 -- not an asteroid (will add it to exclusion list)
22:04:51.38 +36:57:57.2 -- not an asteroid (will add it to exclusion list)
22:06:53.62 +39:49:46.3 -- not an asteroid (will add it to exclusion list)
21:33:24.09 +35:46:28.4 -- not an asteroid (will add it to exclusion list)
21:39:07.59 +35:00:10.2 -- not an asteroid (will add it to exclusion list)
22:12:09.67 +41:33:21.3 -- not an asteroid (will add it to exclusion list)
22:02:21.09 +39:30:31.7 -- not an asteroid (will add it to exclusion list)
21:51:39.74 +34:33:53.1 -- not an asteroid (will add it to exclusion list)
21:27:15.70 +41:14:43.5 -- not an asteroid (will add it to exclusion list)
22:08:05.92 +41:53:33.1 -- not an asteroid (will add it to exclusion list)
21:31:06.96 +36:30:53.1 -- not an asteroid (will add it to exclusion list)
21:58:23.08 +40:16:07.5 -- not an asteroid (will add it to exclusion list)
21:56:24.88 +33:43:30.6 -- not an asteroid (will add it to exclusion list)
21:37:56.98 +36:43:05.2 -- not an asteroid (will add it to exclusion list)
21:54:34.88 +35:47:37.9 -- not an asteroid (will add it to exclusion list)
21:37:46.82 +38:52:30.6 -- not an asteroid (will add it to exclusion list)
21:56:28.84 +40:10:13.7 -- not an asteroid (will add it to exclusion list)
22:07:18.00 +39:07:48.0 -- not an asteroid (will add it to exclusion list)
21:45:58.85 +39:55:47.4 -- not an asteroid (will add it to exclusion list)
21:55:53.88 +37:45:12.7 -- not an asteroid (will add it to exclusion list)
21:33:42.50 +33:41:49.3 -- not an asteroid (will add it to exclusion list)
21:34:53.25 +33:57:00.7 -- not an asteroid (will add it to exclusion list)
22:01:30.88 +34:42:16.9 -- not an asteroid (will add it to exclusion list)
21:39:15.46 +34:56:58.7 -- not an asteroid (will add it to exclusion list)
21:42:21.25 +38:13:06.7 -- not an asteroid (will add it to exclusion list)
21:42:57.35 +37:28:41.7 -- not an asteroid (will add it to exclusion list)
21:31:22.22 +35:13:15.7 -- not an asteroid (will add it to exclusion list)
21:54:19.90 +38:01:39.8 -- not an asteroid (will add it to exclusion list)
21:53:53.39 +38:35:29.4 -- not an asteroid (will add it to exclusion list)
22:03:34.20 +42:00:34.8 -- not an asteroid (will add it to exclusion list)
22:09:18.89 +39:53:05.4 -- not an asteroid (will add it to exclusion list)
21:37:25.90 +37:09:17.8 -- not an asteroid (will add it to exclusion list)
22:06:27.14 +39:09:53.4 -- not an asteroid (will add it to exclusion list)
21:59:50.31 +38:00:40.6 -- not an asteroid (will add it to exclusion list)
21:44:37.99 +36:48:09.0 -- not an asteroid (will add it to exclusion list)
21:55:20.50 +36:22:54.1 -- not an asteroid (will add it to exclusion list)
21:47:08.02 +39:07:42.4 -- not an asteroid (will add it to exclusion list)
21:56:44.92 +37:19:57.3 -- not an asteroid (will add it to exclusion list)
21:36:01.16 +35:40:54.0 -- not an asteroid (will add it to exclusion list)
22:11:07.90 +41:18:47.3 -- not an asteroid (will add it to exclusion list)
21:35:51.51 +40:29:40.4 -- not an asteroid (will add it to exclusion list)
21:50:22.16 +36:49:02.3 -- not an asteroid (will add it to exclusion list)
22:00:11.33 +39:37:40.3 -- not an asteroid (will add it to exclusion list)
21:49:30.71 +36:39:36.7 -- not an asteroid (will add it to exclusion list)
21:40:16.32 +42:12:47.5 -- not an asteroid (will add it to exclusion list)
21:36:08.70 +34:46:10.3 -- not an asteroid (will add it to exclusion list)
21:49:05.03 +37:22:33.2 -- not an asteroid (will add it to exclusion list)
22:04:19.66 +41:12:36.0 -- not an asteroid (will add it to exclusion list)
21:44:48.48 +37:00:33.6 -- not an asteroid (will add it to exclusion list)
21:48:10.19 +38:13:39.2 -- not an asteroid (will add it to exclusion list)
21:32:50.72 +33:42:55.1 -- not an asteroid (will add it to exclusion list)
21:59:59.41 +38:04:06.0 -- not an asteroid (will add it to exclusion list)
21:50:48.59 +40:31:54.5 -- not an asteroid (will add it to exclusion list)
21:38:19.67 +39:47:35.5 -- not an asteroid (will add it to exclusion list)
21:34:44.21 +34:15:39.7 -- not an asteroid (will add it to exclusion list)
21:40:26.00 +37:35:59.3 -- not an asteroid (will add it to exclusion list)
21:31:05.39 +36:09:34.8 -- not an asteroid (will add it to exclusion list)
21:29:09.98 +41:18:07.3 -- not an asteroid (will add it to exclusion list)
21:45:06.46 +36:34:14.0 -- not an asteroid (will add it to exclusion list)
21:58:27.13 +41:39:26.3 -- not an asteroid (will add it to exclusion list)
21:26:40.62 +35:39:06.4 -- not an asteroid (will add it to exclusion list)
21:54:14.47 +37:16:15.6 -- not an asteroid (will add it to exclusion list)
21:51:58.13 +41:43:01.2 -- not an asteroid (will add it to exclusion list)
21:45:18.35 +34:36:18.0 -- not an asteroid (will add it to exclusion list)
21:41:54.81 +36:47:08.4 -- not an asteroid (will add it to exclusion list)
21:29:55.69 +35:17:01.3 -- not an asteroid (will add it to exclusion list)
21:45:41.62 +35:36:34.3 -- not an asteroid (will add it to exclusion list)
21:37:36.08 +34:52:16.3 -- not an asteroid (will add it to exclusion list)
21:35:22.68 +38:34:23.9 -- not an asteroid (will add it to exclusion list)
21:43:00.86 +35:26:44.6 -- not an asteroid (will add it to exclusion list)
21:46:40.74 +34:44:02.8 -- not an asteroid (will add it to exclusion list)
21:42:17.53 +34:59:16.4 -- not an asteroid (will add it to exclusion list)
21:54:33.27 +39:45:07.3 -- not an asteroid (will add it to exclusion list)
21:35:57.20 +34:28:48.1 -- not an asteroid (will add it to exclusion list)
21:52:02.06 +38:59:15.3 -- not an asteroid (will add it to exclusion list)
21:32:42.44 +36:55:39.2 -- not an asteroid (will add it to exclusion list)
21:58:13.02 +41:37:34.2 -- not an asteroid (will add it to exclusion list)
21:30:51.48 +34:08:40.4 -- not an asteroid (will add it to exclusion list)
21:43:08.02 +37:05:00.7 -- not an asteroid (will add it to exclusion list)
21:32:03.99 +37:14:51.8 -- not an asteroid (will add it to exclusion list)
21:47:40.00 +41:28:28.3 -- not an asteroid (will add it to exclusion list)
21:41:56.96 +38:01:50.7 -- not an asteroid (will add it to exclusion list)
21:42:08.11 +39:54:00.0 -- not an asteroid (will add it to exclusion list)
21:28:54.95 +36:35:23.5 -- not an asteroid (will add it to exclusion list)
21:29:37.24 +34:35:10.8 -- not an asteroid (will add it to exclusion list)
21:43:20.90 +38:08:13.2 -- not an asteroid (will add it to exclusion list)
21:27:23.67 +37:00:28.1 -- not an asteroid (will add it to exclusion list)
21:35:04.43 +35:48:29.8 -- not an asteroid (will add it to exclusion list)
21:42:08.14 +41:34:23.5 -- not an asteroid (will add it to exclusion list)
21:39:13.02 +38:06:35.0 -- not an asteroid (will add it to exclusion list)
21:27:01.23 +34:53:28.2 -- not an asteroid (will add it to exclusion list)
21:27:08.97 +35:52:28.6 -- not an asteroid (will add it to exclusion list)
21:32:03.16 +35:39:41.6 -- not an asteroid (will add it to exclusion list)
21:30:23.75 +40:32:52.1 -- not an asteroid (will add it to exclusion list)
21:18:30.76 +41:07:56.6 -- not an asteroid (will add it to exclusion list)
21:26:52.42 +41:39:00.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:18:30.76 +41:07:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:26.98 +37:43:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:40.62 +35:39:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:40.74 +39:52:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:46.13 +37:00:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:51.68 +34:03:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:52.42 +41:39:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.85 +33:43:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:55.25 +38:03:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:00.76 +33:45:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:01.23 +34:53:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:06.61 +33:44:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:07.34 +35:14:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:08.97 +35:52:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:12.50 +33:51:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:14.01 +34:30:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:15.70 +41:14:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:20.05 +35:46:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:23.67 +37:00:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:28.02 +39:54:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:30.62 +35:18:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:56.81 +35:27:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:04.99 +35:56:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.42 +33:41:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:08.29 +36:20:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:09.30 +41:14:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:11.99 +34:45:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:12.79 +36:49:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:13.25 +40:35:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:15.82 +34:43:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:20.93 +36:09:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:22.15 +41:32:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:31.47 +41:22:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.48 +36:04:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.59 +35:11:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.73 +35:42:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:45.26 +36:42:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:54.95 +36:35:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:55.84 +39:02:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.32 +38:59:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.99 +33:49:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:04.98 +34:49:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:05.04 +40:36:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:09.98 +41:18:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:16.00 +34:53:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:16.83 +34:43:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:18.14 +33:38:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:22.39 +34:26:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:24.07 +33:58:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:26.32 +37:55:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:37.24 +34:35:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:38.98 +36:14:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:44.17 +35:02:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:46.34 +35:53:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:55.69 +35:17:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:08.27 +37:30:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:22.42 +38:20:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:23.75 +40:32:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:28.13 +38:52:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:29.91 +39:49:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:30.66 +33:57:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:30.84 +40:52:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:32.04 +35:46:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:33.16 +34:04:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:39.34 +38:36:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:41.28 +35:07:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:51.48 +34:08:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:05.39 +36:09:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:06.96 +36:30:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.97 +38:46:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:17.47 +37:57:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:17.69 +33:40:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:19.68 +39:08:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:22.22 +35:13:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:26.89 +33:46:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:29.68 +33:55:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:31.11 +41:31:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:32.90 +33:56:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:39.39 +36:46:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:40.91 +33:48:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:57.30 +36:19:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:03.16 +35:39:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:03.99 +37:14:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:06.91 +39:41:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:14.37 +37:49:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:18.87 +39:50:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:31.05 +37:13:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:35.91 +35:36:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:38.78 +34:43:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:42.44 +36:55:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:45.10 +38:02:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:50.72 +33:42:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:51.76 +35:15:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:10.28 +41:39:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:11.14 +39:46:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:13.81 +37:12:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:15.00 +33:54:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:16.16 +41:46:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:22.18 +38:02:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:23.27 +35:48:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:24.09 +35:46:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:29.11 +33:39:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:29.30 +37:59:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:31.70 +37:30:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:40.02 +33:37:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:42.50 +33:41:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:43.05 +37:03:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:52.98 +36:12:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:58.57 +36:17:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:02.89 +36:28:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:10.50 +35:44:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:22.92 +34:51:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:28.42 +40:12:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:29.38 +39:23:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:30.55 +33:45:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:31.83 +40:00:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:37.63 +34:15:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:44.21 +34:15:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:45.74 +38:35:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:49.80 +42:03:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:53.25 +33:57:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:54.31 +35:45:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:04.43 +35:48:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:14.10 +35:46:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:21.65 +41:16:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:22.68 +38:34:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:23.86 +34:51:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:24.09 +36:47:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:25.71 +40:25:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:34.13 +34:35:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:35.36 +35:59:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:41.21 +35:13:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:45.33 +33:50:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:46.01 +36:23:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:51.51 +40:29:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:57.20 +34:28:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:57.86 +41:51:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:01.16 +35:40:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:08.38 +34:28:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:08.48 +35:55:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:08.70 +34:46:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:11.19 +38:20:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:13.40 +36:37:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:14.22 +40:15:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:16.89 +35:02:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:23.81 +37:21:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:24.02 +37:34:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:41.98 +36:15:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:49.67 +39:45:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:54.42 +37:55:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:56.43 +36:30:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:57.17 +34:14:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:58.26 +37:51:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:58.91 +34:31:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:02.85 +36:17:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:03.51 +37:31:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:12.18 +40:33:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:13.77 +40:19:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:14.59 +37:16:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:17.02 +36:54:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:25.90 +37:09:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:28.91 +34:32:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:29.63 +35:54:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:32.90 +34:45:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:36.08 +34:52:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.82 +38:52:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.88 +36:44:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:56.98 +36:43:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:58.77 +36:42:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:03.92 +38:03:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:09.32 +36:54:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:15.46 +38:02:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:19.67 +39:47:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:06.45 +37:40:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:07.59 +35:00:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:10.96 +36:29:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:13.02 +38:06:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:15.46 +34:56:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:17.12 +36:38:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:19.17 +36:37:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:23.59 +37:37:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:26.02 +34:58:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:40.95 +34:24:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:50.75 +37:38:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:53.74 +37:58:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.93 +34:16:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:15.60 +37:50:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:16.32 +42:12:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:17.04 +41:25:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:21.22 +39:47:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:26.00 +37:35:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:26.40 +39:27:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:31.53 +37:49:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:34.69 +33:42:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:39.67 +36:27:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:41.05 +36:19:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.84 +37:22:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:44.27 +35:27:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:47.62 +37:32:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:55.51 +35:54:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.14 +41:13:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:04.38 +37:16:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:05.04 +34:50:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:11.94 +41:00:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:32.72 +36:23:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:44.91 +34:02:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:45.31 +37:40:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:54.81 +36:47:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:56.61 +38:52:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:56.96 +38:01:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:57.73 +41:24:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:58.03 +35:21:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:02.26 +37:42:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:08.11 +39:54:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:08.14 +41:34:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:17.53 +34:59:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:21.25 +38:13:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:21.52 +36:16:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:25.14 +35:54:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:26.08 +37:18:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:31.31 +35:51:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:33.81 +41:45:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:39.00 +37:00:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:39.45 +37:40:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:44.12 +39:07:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:51.49 +37:11:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:57.35 +37:28:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:00.86 +35:26:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:02.34 +34:00:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:05.91 +37:32:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:06.26 +37:12:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:08.02 +37:05:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:17.63 +38:29:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:20.61 +36:54:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:20.90 +38:08:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:23.84 +33:45:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:24.22 +39:02:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:24.81 +37:27:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:28.90 +37:46:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:50.45 +37:03:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:01.36 +38:56:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:02.27 +38:24:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:03.17 +37:47:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:09.01 +35:27:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:09.61 +37:55:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:13.05 +38:35:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:23.69 +38:52:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.99 +36:48:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:42.94 +35:29:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:43.69 +35:06:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:48.48 +37:00:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:51.80 +36:12:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:01.35 +40:16:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:02.97 +36:40:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:06.46 +36:34:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:12.02 +40:36:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.29 +37:39:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:18.35 +34:36:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:21.68 +37:55:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:30.14 +42:12:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:30.42 +40:39:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:41.62 +35:36:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:48.52 +34:00:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:54.78 +36:04:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:58.85 +39:55:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:04.46 +34:31:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:11.76 +36:11:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:12.49 +39:34:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:22.62 +36:17:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:35.91 +37:00:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:37.68 +36:31:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:38.91 +34:22:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:40.74 +34:44:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:48.64 +36:53:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:54.04 +39:15:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:56.92 +41:43:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:02.34 +36:41:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:08.02 +39:07:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:12.13 +36:46:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:31.33 +37:36:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:32.63 +41:45:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:33.77 +37:22:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:40.00 +41:28:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:46.25 +35:56:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:46.78 +37:36:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:51.58 +40:21:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:53.10 +34:00:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:08.00 +39:26:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:10.19 +38:13:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:12.58 +41:41:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:15.82 +35:31:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:31.78 +39:16:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:39.22 +37:49:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:40.82 +41:58:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:46.74 +35:26:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.80 +38:52:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.11 +38:28:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:57.95 +37:42:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:03.73 +39:29:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:05.03 +37:22:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:08.07 +35:40:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:09.64 +42:12:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:13.72 +35:11:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:15.19 +35:18:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:19.26 +36:58:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:19.52 +40:40:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:22.29 +41:57:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:25.96 +38:25:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:28.07 +34:19:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:28.23 +38:12:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:30.28 +38:28:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:30.71 +36:39:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:41.31 +37:43:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:59.42 +34:39:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:07.74 +42:10:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:08.02 +34:33:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:17.59 +42:04:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:22.16 +36:49:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:22.68 +40:29:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:25.17 +35:00:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:25.25 +38:28:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:30.82 +36:49:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:34.42 +37:11:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:35.57 +37:36:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:37.07 +36:00:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:38.82 +39:20:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:41.80 +36:02:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:44.44 +36:27:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:48.59 +40:31:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:53.08 +37:38:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:55.25 +34:16:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:56.50 +33:55:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:58.78 +36:44:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:03.23 +33:59:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:03.60 +36:58:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:11.92 +37:00:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:12.70 +35:28:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:22.88 +33:49:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:26.79 +38:24:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:29.81 +37:52:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:31.60 +37:29:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.19 +36:55:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.59 +40:18:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.74 +34:33:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:40.11 +38:49:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:41.99 +34:07:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:47.59 +36:45:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:57.64 +37:11:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:58.13 +41:43:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:02.06 +38:59:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:14.12 +37:49:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:15.43 +41:18:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:19.93 +39:44:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:31.29 +41:07:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:44.60 +34:42:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:45.65 +42:15:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:57.14 +41:56:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:59.24 +34:14:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:00.65 +35:46:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:07.93 +40:37:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:14.97 +36:41:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:18.52 +38:48:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:20.58 +39:06:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:31.10 +33:46:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:31.29 +36:34:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:37.65 +42:15:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:39.07 +34:51:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:41.44 +40:47:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:48.08 +40:18:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:51.27 +33:51:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:53.39 +38:35:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:04.90 +35:09:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:12.72 +35:10:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:13.84 +42:03:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:14.47 +37:16:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:17.40 +36:52:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:19.06 +34:21:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:19.90 +38:01:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:21.74 +42:02:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:25.08 +39:39:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:32.82 +35:25:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:33.27 +39:45:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:34.88 +35:47:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:36.22 +36:42:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:38.60 +36:53:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:39.47 +39:49:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:45.91 +38:18:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:51.04 +40:07:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:53.71 +41:04:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:07.10 +38:37:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:11.88 +36:28:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:19.69 +36:41:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:20.50 +36:22:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:20.84 +34:39:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:27.21 +41:39:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:36.33 +35:51:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:53.68 +42:08:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:53.88 +37:45:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.58 +37:10:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:03.61 +38:29:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:04.82 +37:14:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:15.10 +41:22:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:23.29 +38:47:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:24.88 +33:43:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:26.04 +37:57:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:28.84 +40:10:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:29.42 +36:52:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:34.64 +37:00:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:44.92 +37:19:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:45.81 +40:47:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:52.31 +39:21:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:10.60 +42:10:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:11.29 +40:23:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:12.31 +36:23:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:14.45 +42:01:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:21.05 +35:17:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:21.27 +37:30:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:31.30 +38:48:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:35.09 +40:21:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:38.67 +36:43:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:39.33 +41:47:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:39.47 +41:25:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:44.02 +34:13:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:52.96 +34:06:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:53.26 +36:58:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:00.76 +37:39:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:01.47 +38:57:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:11.17 +38:50:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:13.02 +41:37:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:23.08 +40:16:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:23.87 +37:48:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:26.35 +42:12:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:27.13 +41:39:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:28.78 +40:10:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:32.72 +37:55:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:33.10 +38:59:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:36.26 +41:09:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:37.95 +35:47:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:42.71 +38:46:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:43.33 +42:11:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:43.93 +39:44:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:48.24 +40:45:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:49.54 +40:28:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:52.18 +37:02:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:04.05 +35:55:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:05.04 +35:36:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:06.43 +34:00:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:07.04 +37:35:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:09.95 +36:16:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:17.07 +35:39:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:20.91 +36:56:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:27.03 +41:38:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:28.83 +37:59:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:31.05 +42:08:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:40.08 +41:01:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:42.10 +41:00:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:50.31 +38:00:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:50.53 +41:52:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:54.31 +34:16:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:56.19 +38:33:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:59.23 +36:08:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:59.41 +38:04:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:06.38 +39:09:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:09.65 +33:45:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:10.43 +38:33:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:11.33 +39:37:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:13.35 +34:58:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:13.59 +38:25:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:13.75 +41:45:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:15.80 +35:08:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:16.07 +41:05:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:17.81 +40:36:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:17.84 +38:06:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:20.90 +41:35:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:22.58 +36:02:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:24.33 +35:58:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:24.47 +39:57:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:25.81 +37:57:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:26.34 +35:56:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:37.00 +35:01:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:37.79 +41:43:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:40.88 +34:40:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:45.71 +42:12:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:45.78 +42:12:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:56.16 +36:53:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:04.09 +41:04:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:06.63 +42:14:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:09.64 +39:37:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:12.35 +35:17:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:14.44 +38:33:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:18.69 +41:30:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:20.19 +41:45:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.48 +40:55:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:24.44 +41:55:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:30.08 +41:04:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:30.88 +34:42:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:39.44 +34:45:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:48.10 +38:11:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:48.30 +39:56:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:04.72 +37:45:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:05.34 +37:22:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:05.91 +41:42:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:10.53 +42:07:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:11.40 +35:32:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:13.94 +41:47:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:14.92 +34:37:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:17.99 +35:48:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:20.04 +34:02:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:21.09 +39:30:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.69 +41:34:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:38.99 +37:13:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:41.97 +41:43:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.11 +37:08:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.57 +41:44:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:43.72 +35:30:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:49.10 +35:57:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:54.23 +40:52:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:56.32 +40:46:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:00.73 +38:51:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:02.51 +36:29:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:04.95 +35:09:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:06.42 +40:42:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:08.35 +41:49:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:12.98 +39:06:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:19.33 +33:44:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:19.70 +38:40:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:26.52 +35:25:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:34.20 +42:00:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:38.17 +36:16:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:45.58 +37:16:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:46.20 +38:55:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:59.79 +41:38:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:05.48 +41:13:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:12.58 +40:40:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:19.66 +41:12:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:23.77 +39:34:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:30.32 +41:26:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:34.65 +36:25:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:39.48 +41:55:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:39.71 +37:04:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:41.21 +40:20:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:43.21 +42:01:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:44.36 +37:33:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:46.29 +42:08:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:51.38 +36:57:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:54.69 +35:49:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:59.77 +39:57:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:09.75 +37:59:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:27.15 +41:32:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:27.65 +42:00:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:32.49 +38:58:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:37.45 +38:57:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:37.91 +35:36:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:39.89 +34:53:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:42.70 +35:53:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:48.96 +40:22:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:53.67 +41:23:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:58.50 +41:55:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:02.05 +40:00:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:02.53 +38:59:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:05.56 +41:38:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:09.41 +39:56:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:12.37 +39:36:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:13.56 +41:38:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:23.77 +41:39:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:24.16 +38:41:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:27.14 +39:09:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:28.76 +39:03:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:29.11 +39:32:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:30.62 +34:18:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:31.92 +34:33:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:37.68 +41:44:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:38.72 +41:43:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:41.13 +40:11:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:42.48 +40:57:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:53.62 +39:49:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:56.78 +36:48:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:02.72 +41:57:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:10.96 +38:37:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:12.31 +41:10:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:18.00 +39:07:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:22.71 +40:35:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:23.06 +41:08:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:31.14 +39:46:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:35.18 +41:27:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:43.41 +37:37:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:48.92 +34:48:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:52.46 +41:59:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:53.03 +37:40:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:01.57 +35:58:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:02.15 +37:33:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:05.92 +41:53:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:10.70 +39:02:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:12.38 +39:44:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:21.44 +34:16:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:28.16 +41:17:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:28.75 +34:30:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:34.63 +37:33:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:43.68 +41:30:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:49.92 +40:21:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:55.68 +38:16:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:56.95 +41:29:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:57.22 +36:50:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:58.89 +42:02:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:10.00 +41:58:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:10.52 +33:47:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.66 +36:46:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:13.59 +39:15:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:18.89 +39:53:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:33.65 +41:54:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:46.32 +41:39:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:51.75 +41:55:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:55.37 +40:48:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:59.93 +38:20:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:02.92 +36:44:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:06.42 +35:55:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:14.91 +41:02:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:15.85 +41:34:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:20.20 +38:44:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:20.81 +41:33:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:32.03 +41:45:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:36.56 +39:03:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:43.52 +41:09:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:57.04 +37:02:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:02.23 +38:11:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:07.15 +41:20:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:07.90 +41:18:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:12.81 +41:39:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:31.18 +40:27:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:35.58 +41:59:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:43.30 +42:07:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:45.13 +41:45:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:50.18 +39:03:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:52.00 +42:03:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:52.66 +40:52:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:02.15 +41:01:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:04.92 +39:17:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:09.67 +41:33:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:24.03 +40:35:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
21:18:30.76 +41:07:56.6 -- a known variable star
21:26:26.98 +37:43:49.9 -- not a known variable star
21:26:40.62 +35:39:06.4 -- a known variable star
21:26:40.74 +39:52:49.0 -- a known variable star
21:26:46.13 +37:00:02.7 -- not a known variable star
21:26:51.68 +34:03:09.6 -- a known variable star
21:26:52.42 +41:39:00.1 -- a known variable star
21:26:53.85 +33:43:13.3 -- not a known variable star
21:26:55.25 +38:03:55.3 -- not a known variable star
21:27:00.76 +33:45:02.8 -- not a known variable star
21:27:01.23 +34:53:28.2 -- not a known variable star
21:27:06.61 +33:44:10.1 -- a known variable star
21:27:07.34 +35:14:58.4 -- not a known variable star
21:27:08.97 +35:52:28.6 -- a known variable star
21:27:12.50 +33:51:25.4 -- not a known variable star
21:27:14.01 +34:30:08.1 -- not a known variable star
21:27:15.70 +41:14:43.5 -- not a known variable star
21:27:20.05 +35:46:48.2 -- not a known variable star
21:27:23.67 +37:00:28.1 -- not a known variable star
21:27:28.02 +39:54:38.6 -- not a known variable star
21:27:30.62 +35:18:41.9 -- not a known variable star
21:27:56.81 +35:27:16.8 -- a known variable star
21:28:04.99 +35:56:21.6 -- not a known variable star
21:28:06.42 +33:41:27.0 -- not a known variable star
21:28:08.29 +36:20:37.2 -- not a known variable star
21:28:09.30 +41:14:37.1 -- not a known variable star
21:28:11.99 +34:45:25.7 -- not a known variable star
21:28:12.79 +36:49:25.2 -- not a known variable star
21:28:13.25 +40:35:50.7 -- not a known variable star
21:28:15.82 +34:43:42.3 -- not a known variable star
21:28:20.93 +36:09:00.3 -- not a known variable star
21:28:22.15 +41:32:00.3 -- not a known variable star
21:28:31.47 +41:22:58.2 -- not a known variable star
21:28:43.48 +36:04:03.7 -- not a known variable star
21:28:43.59 +35:11:02.7 -- a known variable star
21:28:43.73 +35:42:02.4 -- not a known variable star
21:28:45.26 +36:42:07.2 -- not a known variable star
21:28:54.95 +36:35:23.5 -- not a known variable star
21:28:55.84 +39:02:12.2 -- not a known variable star
21:29:00.32 +38:59:30.2 -- not a known variable star
21:29:00.99 +33:49:52.9 -- a known variable star
21:29:04.98 +34:49:01.3 -- not a known variable star
21:29:05.04 +40:36:55.7 -- not a known variable star
21:29:09.98 +41:18:07.3 -- a known variable star
21:29:16.00 +34:53:37.5 -- not a known variable star
21:29:16.83 +34:43:07.0 -- not a known variable star
21:29:18.14 +33:38:40.5 -- not a known variable star
21:29:22.39 +34:26:40.6 -- not a known variable star
21:29:24.07 +33:58:30.2 -- not a known variable star
21:29:26.32 +37:55:00.9 -- not a known variable star
21:29:37.24 +34:35:10.8 -- a known variable star
21:29:38.98 +36:14:25.4 -- not a known variable star
21:29:44.17 +35:02:48.4 -- not a known variable star
21:29:46.34 +35:53:26.3 -- not a known variable star
21:29:55.69 +35:17:01.3 -- a known variable star
21:30:08.27 +37:30:28.0 -- not a known variable star
21:30:22.42 +38:20:38.9 -- not a known variable star
21:30:23.75 +40:32:52.1 -- not a known variable star
21:30:28.13 +38:52:35.3 -- not a known variable star
21:30:29.91 +39:49:30.6 -- a known variable star
21:30:30.66 +33:57:26.0 -- not a known variable star
21:30:30.84 +40:52:58.5 -- not a known variable star
21:30:32.04 +35:46:44.4 -- not a known variable star
21:30:33.16 +34:04:09.8 -- not a known variable star
21:30:39.34 +38:36:14.0 -- not a known variable star
21:30:41.28 +35:07:19.3 -- not a known variable star
21:30:51.48 +34:08:40.4 -- not a known variable star
21:31:05.39 +36:09:34.8 -- not a known variable star
21:31:06.96 +36:30:53.1 -- not a known variable star
21:31:14.97 +38:46:29.7 -- a known variable star
21:31:17.47 +37:57:30.7 -- not a known variable star
21:31:17.69 +33:40:29.1 -- not a known variable star
21:31:19.68 +39:08:30.9 -- a known variable star
21:31:22.22 +35:13:15.7 -- a known variable star
21:31:26.89 +33:46:05.5 -- not a known variable star
21:31:29.68 +33:55:39.8 -- not a known variable star
21:31:31.11 +41:31:49.7 -- not a known variable star
21:31:32.90 +33:56:49.8 -- not a known variable star
21:31:39.39 +36:46:29.2 -- not a known variable star
21:31:40.91 +33:48:11.1 -- not a known variable star
21:31:57.30 +36:19:02.3 -- not a known variable star
21:32:03.16 +35:39:41.6 -- not a known variable star
21:32:03.99 +37:14:51.8 -- not a known variable star
21:32:06.91 +39:41:52.6 -- not a known variable star
21:32:14.37 +37:49:10.6 -- not a known variable star
21:32:18.87 +39:50:34.0 -- not a known variable star
21:32:31.05 +37:13:03.8 -- not a known variable star
21:32:35.91 +35:36:09.9 -- not a known variable star
21:32:38.78 +34:43:55.9 -- not a known variable star
21:32:42.44 +36:55:39.2 -- not a known variable star
21:32:45.10 +38:02:03.6 -- not a known variable star
21:32:50.72 +33:42:55.1 -- not a known variable star
21:32:51.76 +35:15:25.9 -- not a known variable star
21:33:10.28 +41:39:56.3 -- not a known variable star
21:33:11.14 +39:46:10.4 -- a known variable star
21:33:13.81 +37:12:44.0 -- not a known variable star
21:33:15.00 +33:54:30.0 -- not a known variable star
21:33:16.16 +41:46:48.3 -- not a known variable star
21:33:22.18 +38:02:28.7 -- a known variable star
21:33:23.27 +35:48:05.1 -- not a known variable star
21:33:24.09 +35:46:28.4 -- not a known variable star
21:33:29.11 +33:39:19.5 -- not a known variable star
21:33:29.30 +37:59:54.7 -- a known variable star
21:33:31.70 +37:30:03.8 -- not a known variable star
21:33:40.02 +33:37:46.0 -- not a known variable star
21:33:42.50 +33:41:49.3 -- not a known variable star
21:33:43.05 +37:03:45.6 -- not a known variable star
21:33:52.98 +36:12:28.2 -- not a known variable star
21:33:58.57 +36:17:17.8 -- not a known variable star
21:34:02.89 +36:28:38.6 -- not a known variable star
21:34:10.50 +35:44:49.6 -- not a known variable star
21:34:22.92 +34:51:23.4 -- not a known variable star
21:34:28.42 +40:12:23.8 -- not a known variable star
21:34:29.38 +39:23:38.8 -- not a known variable star
21:34:30.55 +33:45:42.3 -- not a known variable star
21:34:31.83 +40:00:34.5 -- not a known variable star
21:34:37.63 +34:15:56.3 -- not a known variable star
21:34:44.21 +34:15:39.7 -- not a known variable star
21:34:45.74 +38:35:14.3 -- not a known variable star
21:34:49.80 +42:03:15.4 -- not a known variable star
21:34:53.25 +33:57:00.7 -- a known variable star
21:34:54.31 +35:45:43.1 -- not a known variable star
21:35:04.43 +35:48:29.8 -- a known variable star
21:35:14.10 +35:46:26.8 -- not a known variable star
21:35:21.65 +41:16:19.3 -- not a known variable star
21:35:22.68 +38:34:23.9 -- not a known variable star
21:35:23.86 +34:51:32.9 -- not a known variable star
21:35:24.09 +36:47:16.4 -- not a known variable star
21:35:25.71 +40:25:30.5 -- not a known variable star
21:35:34.13 +34:35:52.2 -- not a known variable star
21:35:35.36 +35:59:26.5 -- not a known variable star
21:35:41.21 +35:13:20.9 -- a known variable star
21:35:45.33 +33:50:35.9 -- not a known variable star
21:35:46.01 +36:23:43.6 -- not a known variable star
21:35:51.51 +40:29:40.4 -- a known variable star
21:35:57.20 +34:28:48.1 -- not a known variable star
21:35:57.86 +41:51:55.7 -- a known variable star
21:36:01.16 +35:40:54.0 -- not a known variable star
21:36:08.38 +34:28:55.9 -- not a known variable star
21:36:08.48 +35:55:06.2 -- not a known variable star
21:36:08.70 +34:46:10.3 -- not a known variable star
21:36:11.19 +38:20:58.6 -- not a known variable star
21:36:13.40 +36:37:41.9 -- not a known variable star
21:36:14.22 +40:15:40.1 -- not a known variable star
21:36:16.89 +35:02:27.0 -- not a known variable star
21:36:23.81 +37:21:33.7 -- a known variable star
21:36:24.02 +37:34:32.2 -- not a known variable star
21:36:41.98 +36:15:49.7 -- a known variable star
21:36:49.67 +39:45:20.6 -- not a known variable star
21:36:54.42 +37:55:38.1 -- not a known variable star
21:36:56.43 +36:30:10.2 -- a known variable star
21:36:57.17 +34:14:37.0 -- a known variable star
21:36:58.26 +37:51:36.1 -- not a known variable star
21:36:58.91 +34:31:59.2 -- not a known variable star
21:37:02.85 +36:17:37.9 -- not a known variable star
21:37:03.51 +37:31:36.8 -- not a known variable star
21:37:12.18 +40:33:58.9 -- not a known variable star
21:37:13.77 +40:19:25.1 -- not a known variable star
21:37:14.59 +37:16:14.3 -- not a known variable star
21:37:17.02 +36:54:05.4 -- not a known variable star
21:37:25.90 +37:09:17.8 -- not a known variable star
21:37:28.91 +34:32:02.1 -- not a known variable star
21:37:29.63 +35:54:14.5 -- not a known variable star
21:37:32.90 +34:45:17.1 -- not a known variable star
21:37:36.08 +34:52:16.3 -- not a known variable star
21:37:46.82 +38:52:30.6 -- not a known variable star
21:37:46.88 +36:44:34.4 -- a known variable star
21:37:56.98 +36:43:05.2 -- not a known variable star
21:37:58.77 +36:42:07.1 -- not a known variable star
21:38:03.92 +38:03:50.8 -- not a known variable star
21:38:09.32 +36:54:28.0 -- not a known variable star
21:38:15.46 +38:02:08.4 -- not a known variable star
21:38:19.67 +39:47:35.5 -- not a known variable star
21:39:06.45 +37:40:27.9 -- not a known variable star
21:39:07.59 +35:00:10.2 -- not a known variable star
21:39:10.96 +36:29:08.3 -- not a known variable star
21:39:13.02 +38:06:35.0 -- not a known variable star
21:39:15.46 +34:56:58.7 -- not a known variable star
21:39:17.12 +36:38:31.8 -- not a known variable star
21:39:19.17 +36:37:29.1 -- not a known variable star
21:39:23.59 +37:37:07.9 -- not a known variable star
21:39:26.02 +34:58:46.9 -- not a known variable star
21:39:40.95 +34:24:59.2 -- not a known variable star
21:39:50.75 +37:38:28.6 -- not a known variable star
21:39:53.74 +37:58:53.1 -- not a known variable star
21:40:12.93 +34:16:54.1 -- not a known variable star
21:40:15.60 +37:50:20.1 -- not a known variable star
21:40:16.32 +42:12:47.5 -- a known variable star
21:40:17.04 +41:25:00.8 -- not a known variable star
21:40:21.22 +39:47:14.7 -- not a known variable star
21:40:26.00 +37:35:59.3 -- not a known variable star
21:40:26.40 +39:27:29.0 -- not a known variable star
21:40:31.53 +37:49:27.5 -- not a known variable star
21:40:34.69 +33:42:27.1 -- not a known variable star
21:40:39.67 +36:27:52.9 -- a known variable star
21:40:41.05 +36:19:20.5 -- not a known variable star
21:40:43.84 +37:22:59.4 -- not a known variable star
21:40:44.27 +35:27:41.7 -- not a known variable star
21:40:47.62 +37:32:56.2 -- not a known variable star
21:40:55.51 +35:54:46.3 -- not a known variable star
21:40:56.14 +41:13:20.7 -- not a known variable star
21:41:04.38 +37:16:08.3 -- not a known variable star
21:41:05.04 +34:50:47.1 -- not a known variable star
21:41:11.94 +41:00:50.9 -- not a known variable star
21:41:32.72 +36:23:15.4 -- not a known variable star
21:41:44.91 +34:02:40.1 -- not a known variable star
21:41:45.31 +37:40:53.2 -- not a known variable star
21:41:54.81 +36:47:08.4 -- not a known variable star
21:41:56.61 +38:52:29.8 -- not a known variable star
21:41:56.96 +38:01:50.7 -- not a known variable star
21:41:57.73 +41:24:19.5 -- not a known variable star
21:41:58.03 +35:21:26.8 -- not a known variable star
21:42:02.26 +37:42:53.1 -- not a known variable star
21:42:08.11 +39:54:00.0 -- not a known variable star
21:42:08.14 +41:34:23.5 -- a known variable star
21:42:17.53 +34:59:16.4 -- not a known variable star
21:42:21.25 +38:13:06.7 -- not a known variable star
21:42:21.52 +36:16:15.6 -- not a known variable star
21:42:25.14 +35:54:12.6 -- not a known variable star
21:42:26.08 +37:18:12.6 -- a known variable star
21:42:31.31 +35:51:14.4 -- not a known variable star
21:42:33.81 +41:45:50.4 -- not a known variable star
21:42:39.00 +37:00:24.2 -- a known variable star
21:42:39.45 +37:40:34.5 -- not a known variable star
21:42:44.12 +39:07:51.7 -- not a known variable star
21:42:51.49 +37:11:24.5 -- not a known variable star
21:42:57.35 +37:28:41.7 -- not a known variable star
21:43:00.86 +35:26:44.6 -- not a known variable star
21:43:02.34 +34:00:48.1 -- not a known variable star
21:43:05.91 +37:32:44.3 -- not a known variable star
21:43:06.26 +37:12:23.6 -- not a known variable star
21:43:08.02 +37:05:00.7 -- a known variable star
21:43:17.63 +38:29:48.8 -- not a known variable star
21:43:20.61 +36:54:41.3 -- a known variable star
21:43:20.90 +38:08:13.2 -- a known variable star
21:43:23.84 +33:45:14.5 -- not a known variable star
21:43:24.22 +39:02:44.7 -- not a known variable star
21:43:24.81 +37:27:40.2 -- not a known variable star
21:43:28.90 +37:46:48.1 -- a known variable star
21:43:50.45 +37:03:22.9 -- not a known variable star
21:44:01.36 +38:56:13.3 -- not a known variable star
21:44:02.27 +38:24:38.7 -- a known variable star
21:44:03.17 +37:47:35.8 -- not a known variable star
21:44:09.01 +35:27:53.6 -- a known variable star
21:44:09.61 +37:55:02.7 -- not a known variable star
21:44:13.05 +38:35:36.7 -- not a known variable star
21:44:23.69 +38:52:48.1 -- not a known variable star
21:44:37.99 +36:48:09.0 -- not a known variable star
21:44:42.94 +35:29:07.5 -- a known variable star
21:44:43.69 +35:06:39.2 -- not a known variable star
21:44:48.48 +37:00:33.6 -- not a known variable star
21:44:51.80 +36:12:12.5 -- not a known variable star
21:45:01.35 +40:16:55.6 -- not a known variable star
21:45:02.97 +36:40:08.0 -- not a known variable star
21:45:06.46 +36:34:14.0 -- not a known variable star
21:45:12.02 +40:36:35.5 -- not a known variable star
21:45:18.29 +37:39:34.8 -- not a known variable star
21:45:18.35 +34:36:18.0 -- not a known variable star
21:45:21.68 +37:55:18.5 -- not a known variable star
21:45:30.14 +42:12:25.2 -- a known variable star
21:45:30.42 +40:39:22.2 -- not a known variable star
21:45:41.62 +35:36:34.3 -- not a known variable star
21:45:48.52 +34:00:26.9 -- not a known variable star
21:45:54.78 +36:04:45.0 -- not a known variable star
21:45:58.85 +39:55:47.4 -- a known variable star
21:46:04.46 +34:31:28.8 -- not a known variable star
21:46:11.76 +36:11:01.7 -- not a known variable star
21:46:12.49 +39:34:00.4 -- not a known variable star
21:46:22.62 +36:17:37.7 -- not a known variable star
21:46:35.91 +37:00:51.7 -- not a known variable star
21:46:37.68 +36:31:34.8 -- not a known variable star
21:46:38.91 +34:22:59.8 -- not a known variable star
21:46:40.74 +34:44:02.8 -- not a known variable star
21:46:48.64 +36:53:20.3 -- not a known variable star
21:46:54.04 +39:15:19.9 -- not a known variable star
21:46:56.92 +41:43:39.2 -- not a known variable star
21:47:02.34 +36:41:21.7 -- a known variable star
21:47:08.02 +39:07:42.4 -- a known variable star
21:47:12.13 +36:46:39.3 -- not a known variable star
21:47:31.33 +37:36:09.6 -- not a known variable star
21:47:32.63 +41:45:11.6 -- not a known variable star
21:47:33.77 +37:22:55.8 -- not a known variable star
21:47:40.00 +41:28:28.3 -- not a known variable star
21:47:46.25 +35:56:49.8 -- not a known variable star
21:47:46.78 +37:36:30.0 -- not a known variable star
21:47:51.58 +40:21:48.5 -- not a known variable star
21:47:53.10 +34:00:34.1 -- not a known variable star
21:48:08.00 +39:26:18.8 -- not a known variable star
21:48:10.19 +38:13:39.2 -- not a known variable star
21:48:12.58 +41:41:12.5 -- not a known variable star
21:48:15.82 +35:31:04.0 -- not a known variable star
21:48:31.78 +39:16:35.8 -- not a known variable star
21:48:39.22 +37:49:35.3 -- not a known variable star
21:48:40.82 +41:58:41.0 -- not a known variable star
21:48:46.74 +35:26:20.4 -- not a known variable star
21:48:47.80 +38:52:57.8 -- not a known variable star
21:48:57.11 +38:28:35.3 -- not a known variable star
21:48:57.95 +37:42:52.3 -- not a known variable star
21:49:03.73 +39:29:38.9 -- not a known variable star
21:49:05.03 +37:22:33.2 -- not a known variable star
21:49:08.07 +35:40:21.4 -- not a known variable star
21:49:09.64 +42:12:56.5 -- not a known variable star
21:49:13.72 +35:11:21.8 -- not a known variable star
21:49:15.19 +35:18:21.5 -- not a known variable star
21:49:19.26 +36:58:39.0 -- a known variable star
21:49:19.52 +40:40:24.4 -- not a known variable star
21:49:22.29 +41:57:46.4 -- not a known variable star
21:49:25.96 +38:25:18.2 -- not a known variable star
21:49:28.07 +34:19:21.2 -- not a known variable star
21:49:28.23 +38:12:27.0 -- not a known variable star
21:49:30.28 +38:28:52.1 -- not a known variable star
21:49:30.71 +36:39:36.7 -- a known variable star
21:49:41.31 +37:43:29.6 -- not a known variable star
21:49:59.42 +34:39:56.9 -- not a known variable star
21:50:07.74 +42:10:51.9 -- not a known variable star
21:50:08.02 +34:33:28.4 -- a known variable star
21:50:17.59 +42:04:56.5 -- a known variable star
21:50:22.16 +36:49:02.3 -- not a known variable star
21:50:22.68 +40:29:52.1 -- not a known variable star
21:50:25.17 +35:00:16.6 -- not a known variable star
21:50:25.25 +38:28:29.4 -- not a known variable star
21:50:30.82 +36:49:51.1 -- not a known variable star
21:50:34.42 +37:11:03.5 -- not a known variable star
21:50:35.57 +37:36:20.8 -- not a known variable star
21:50:37.07 +36:00:47.8 -- not a known variable star
21:50:38.82 +39:20:18.3 -- not a known variable star
21:50:41.80 +36:02:33.6 -- a known variable star
21:50:44.44 +36:27:35.4 -- not a known variable star
21:50:48.59 +40:31:54.5 -- not a known variable star
21:50:53.08 +37:38:05.3 -- a known variable star
21:50:55.25 +34:16:15.5 -- not a known variable star
21:50:56.50 +33:55:09.6 -- a known variable star
21:50:58.78 +36:44:37.4 -- not a known variable star
21:51:03.23 +33:59:27.0 -- not a known variable star
21:51:03.60 +36:58:53.3 -- not a known variable star
21:51:11.92 +37:00:41.8 -- not a known variable star
21:51:12.70 +35:28:48.9 -- not a known variable star
21:51:22.88 +33:49:09.9 -- not a known variable star
21:51:26.79 +38:24:24.2 -- not a known variable star
21:51:29.81 +37:52:05.2 -- not a known variable star
21:51:31.60 +37:29:39.0 -- not a known variable star
21:51:39.19 +36:55:28.8 -- not a known variable star
21:51:39.59 +40:18:36.0 -- not a known variable star
21:51:39.74 +34:33:53.1 -- not a known variable star
21:51:40.11 +38:49:49.1 -- not a known variable star
21:51:41.99 +34:07:03.5 -- not a known variable star
21:51:47.59 +36:45:22.7 -- not a known variable star
21:51:57.64 +37:11:55.0 -- not a known variable star
21:51:58.13 +41:43:01.2 -- not a known variable star
21:52:02.06 +38:59:15.3 -- not a known variable star
21:52:14.12 +37:49:46.3 -- not a known variable star
21:52:15.43 +41:18:16.1 -- not a known variable star
21:52:19.93 +39:44:46.8 -- not a known variable star
21:52:31.29 +41:07:39.3 -- not a known variable star
21:52:44.60 +34:42:49.6 -- not a known variable star
21:52:45.65 +42:15:35.3 -- not a known variable star
21:52:57.14 +41:56:24.0 -- not a known variable star
21:52:59.24 +34:14:49.0 -- not a known variable star
21:53:00.65 +35:46:13.8 -- not a known variable star
21:53:07.93 +40:37:52.5 -- not a known variable star
21:53:14.97 +36:41:36.6 -- not a known variable star
21:53:18.52 +38:48:06.9 -- a known variable star
21:53:20.58 +39:06:18.6 -- not a known variable star
21:53:31.10 +33:46:49.4 -- a known variable star
21:53:31.29 +36:34:23.1 -- a known variable star
21:53:37.65 +42:15:49.5 -- a known variable star
21:53:39.07 +34:51:16.0 -- not a known variable star
21:53:41.44 +40:47:14.5 -- not a known variable star
21:53:48.08 +40:18:26.1 -- not a known variable star
21:53:51.27 +33:51:00.5 -- not a known variable star
21:53:53.39 +38:35:29.4 -- not a known variable star
21:54:04.90 +35:09:18.4 -- not a known variable star
21:54:12.72 +35:10:05.1 -- not a known variable star
21:54:13.84 +42:03:14.7 -- not a known variable star
21:54:14.47 +37:16:15.6 -- not a known variable star
21:54:17.40 +36:52:10.6 -- not a known variable star
21:54:19.06 +34:21:38.0 -- not a known variable star
21:54:19.90 +38:01:39.8 -- not a known variable star
21:54:21.74 +42:02:06.9 -- not a known variable star
21:54:25.08 +39:39:28.0 -- not a known variable star
21:54:32.82 +35:25:31.7 -- not a known variable star
21:54:33.27 +39:45:07.3 -- not a known variable star
21:54:34.88 +35:47:37.9 -- not a known variable star
21:54:36.22 +36:42:13.8 -- not a known variable star
21:54:38.60 +36:53:53.5 -- a known variable star
21:54:39.47 +39:49:48.7 -- not a known variable star
21:54:45.91 +38:18:19.5 -- not a known variable star
21:54:51.04 +40:07:59.2 -- a known variable star
21:54:53.71 +41:04:43.2 -- not a known variable star
21:55:07.10 +38:37:59.5 -- not a known variable star
21:55:11.88 +36:28:56.0 -- not a known variable star
21:55:19.69 +36:41:47.8 -- not a known variable star
21:55:20.50 +36:22:54.1 -- not a known variable star
21:55:20.84 +34:39:46.5 -- not a known variable star
21:55:27.21 +41:39:30.1 -- a known variable star
21:55:36.33 +35:51:32.4 -- not a known variable star
21:55:53.68 +42:08:36.5 -- a known variable star
21:55:53.88 +37:45:12.7 -- not a known variable star
21:56:00.58 +37:10:57.1 -- not a known variable star
21:56:03.61 +38:29:55.7 -- not a known variable star
21:56:04.82 +37:14:36.4 -- not a known variable star
21:56:15.10 +41:22:11.4 -- not a known variable star
21:56:23.29 +38:47:33.2 -- not a known variable star
21:56:24.88 +33:43:30.6 -- a known variable star
21:56:26.04 +37:57:07.1 -- not a known variable star
21:56:28.84 +40:10:13.7 -- not a known variable star
21:56:29.42 +36:52:34.4 -- not a known variable star
21:56:34.64 +37:00:25.7 -- not a known variable star
21:56:44.92 +37:19:57.3 -- not a known variable star
21:56:45.81 +40:47:17.0 -- not a known variable star
21:56:52.31 +39:21:22.0 -- not a known variable star
21:57:10.60 +42:10:41.6 -- not a known variable star
21:57:11.29 +40:23:42.7 -- a known variable star
21:57:12.31 +36:23:41.2 -- not a known variable star
21:57:14.45 +42:01:03.9 -- not a known variable star
21:57:21.05 +35:17:18.2 -- a known variable star
21:57:21.27 +37:30:14.8 -- not a known variable star
21:57:31.30 +38:48:28.0 -- not a known variable star
21:57:35.09 +40:21:27.2 -- not a known variable star
21:57:38.67 +36:43:41.1 -- not a known variable star
21:57:39.33 +41:47:18.3 -- not a known variable star
21:57:39.47 +41:25:20.3 -- not a known variable star
21:57:44.02 +34:13:27.3 -- not a known variable star
21:57:52.96 +34:06:45.3 -- not a known variable star
21:57:53.26 +36:58:24.0 -- not a known variable star
21:58:00.76 +37:39:30.9 -- not a known variable star
21:58:01.47 +38:57:27.0 -- not a known variable star
21:58:11.17 +38:50:11.7 -- a known variable star
21:58:13.02 +41:37:34.2 -- not a known variable star
21:58:23.08 +40:16:07.5 -- not a known variable star
21:58:23.87 +37:48:10.5 -- not a known variable star
21:58:26.35 +42:12:16.4 -- not a known variable star
21:58:27.13 +41:39:26.3 -- not a known variable star
21:58:28.78 +40:10:17.0 -- not a known variable star
21:58:32.72 +37:55:01.1 -- not a known variable star
21:58:33.10 +38:59:49.3 -- not a known variable star
21:58:36.26 +41:09:23.1 -- not a known variable star
21:58:37.95 +35:47:12.2 -- not a known variable star
21:58:42.71 +38:46:43.2 -- not a known variable star
21:58:43.33 +42:11:57.9 -- not a known variable star
21:58:43.93 +39:44:49.6 -- not a known variable star
21:58:48.24 +40:45:27.6 -- not a known variable star
21:58:49.54 +40:28:43.1 -- not a known variable star
21:58:52.18 +37:02:33.4 -- not a known variable star
21:59:04.05 +35:55:55.0 -- not a known variable star
21:59:05.04 +35:36:42.6 -- not a known variable star
21:59:06.43 +34:00:17.5 -- not a known variable star
21:59:07.04 +37:35:41.8 -- not a known variable star
21:59:09.95 +36:16:48.9 -- not a known variable star
21:59:17.07 +35:39:25.5 -- not a known variable star
21:59:20.91 +36:56:49.2 -- not a known variable star
21:59:27.03 +41:38:40.6 -- not a known variable star
21:59:28.83 +37:59:48.3 -- not a known variable star
21:59:31.05 +42:08:24.3 -- not a known variable star
21:59:40.08 +41:01:41.0 -- not a known variable star
21:59:42.10 +41:00:46.6 -- not a known variable star
21:59:50.31 +38:00:40.6 -- not a known variable star
21:59:50.53 +41:52:08.1 -- not a known variable star
21:59:54.31 +34:16:50.9 -- not a known variable star
21:59:56.19 +38:33:11.5 -- a known variable star
21:59:59.23 +36:08:33.3 -- not a known variable star
21:59:59.41 +38:04:06.0 -- not a known variable star
22:00:06.38 +39:09:22.8 -- not a known variable star
22:00:09.65 +33:45:56.1 -- not a known variable star
22:00:10.43 +38:33:13.9 -- not a known variable star
22:00:11.33 +39:37:40.3 -- not a known variable star
22:00:13.35 +34:58:25.7 -- not a known variable star
22:00:13.59 +38:25:18.0 -- not a known variable star
22:00:13.75 +41:45:18.1 -- not a known variable star
22:00:15.80 +35:08:28.9 -- not a known variable star
22:00:16.07 +41:05:52.9 -- not a known variable star
22:00:17.81 +40:36:29.5 -- not a known variable star
22:00:17.84 +38:06:34.9 -- not a known variable star
22:00:20.90 +41:35:27.5 -- a known variable star
22:00:22.58 +36:02:18.8 -- not a known variable star
22:00:24.33 +35:58:53.7 -- not a known variable star
22:00:24.47 +39:57:06.7 -- a known variable star
22:00:25.81 +37:57:32.4 -- not a known variable star
22:00:26.34 +35:56:03.5 -- a known variable star
22:00:37.00 +35:01:34.4 -- not a known variable star
22:00:37.79 +41:43:04.1 -- not a known variable star
22:00:40.88 +34:40:45.0 -- not a known variable star
22:00:45.71 +42:12:57.5 -- not a known variable star
22:00:45.78 +42:12:40.6 -- not a known variable star
22:00:56.16 +36:53:36.2 -- not a known variable star
22:01:04.09 +41:04:55.5 -- a known variable star
22:01:06.63 +42:14:36.5 -- not a known variable star
22:01:09.64 +39:37:09.0 -- not a known variable star
22:01:12.35 +35:17:06.2 -- not a known variable star
22:01:14.44 +38:33:47.4 -- not a known variable star
22:01:18.69 +41:30:27.6 -- not a known variable star
22:01:20.19 +41:45:32.7 -- a known variable star
22:01:22.48 +40:55:08.5 -- not a known variable star
22:01:24.44 +41:55:51.4 -- a known variable star
22:01:30.08 +41:04:28.8 -- a known variable star
22:01:30.88 +34:42:16.9 -- not a known variable star
22:01:39.44 +34:45:27.5 -- not a known variable star
22:01:48.10 +38:11:19.5 -- not a known variable star
22:01:48.30 +39:56:07.0 -- not a known variable star
22:02:04.72 +37:45:26.3 -- not a known variable star
22:02:05.34 +37:22:23.9 -- not a known variable star
22:02:05.91 +41:42:42.0 -- not a known variable star
22:02:10.53 +42:07:01.9 -- not a known variable star
22:02:11.40 +35:32:41.6 -- not a known variable star
22:02:13.94 +41:47:07.6 -- not a known variable star
22:02:14.92 +34:37:08.3 -- not a known variable star
22:02:17.99 +35:48:05.0 -- not a known variable star
22:02:20.04 +34:02:55.5 -- not a known variable star
22:02:21.09 +39:30:31.7 -- not a known variable star
22:02:22.69 +41:34:47.5 -- not a known variable star
22:02:38.99 +37:13:44.3 -- not a known variable star
22:02:41.97 +41:43:44.0 -- not a known variable star
22:02:42.11 +37:08:59.4 -- not a known variable star
22:02:42.57 +41:44:09.7 -- not a known variable star
22:02:43.72 +35:30:17.9 -- a known variable star
22:02:49.10 +35:57:04.6 -- not a known variable star
22:02:54.23 +40:52:40.1 -- not a known variable star
22:02:56.32 +40:46:06.8 -- not a known variable star
22:03:00.73 +38:51:52.9 -- not a known variable star
22:03:02.51 +36:29:37.6 -- not a known variable star
22:03:04.95 +35:09:33.5 -- not a known variable star
22:03:06.42 +40:42:37.9 -- not a known variable star
22:03:08.35 +41:49:49.0 -- not a known variable star
22:03:12.98 +39:06:03.2 -- not a known variable star
22:03:19.33 +33:44:47.9 -- not a known variable star
22:03:19.70 +38:40:39.2 -- not a known variable star
22:03:26.52 +35:25:29.3 -- not a known variable star
22:03:34.20 +42:00:34.8 -- not a known variable star
22:03:38.17 +36:16:08.0 -- not a known variable star
22:03:45.58 +37:16:45.0 -- not a known variable star
22:03:46.20 +38:55:41.6 -- not a known variable star
22:03:59.79 +41:38:51.3 -- not a known variable star
22:04:05.48 +41:13:37.3 -- not a known variable star
22:04:12.58 +40:40:22.1 -- not a known variable star
22:04:19.66 +41:12:36.0 -- not a known variable star
22:04:23.77 +39:34:05.5 -- not a known variable star
22:04:30.32 +41:26:44.7 -- not a known variable star
22:04:34.65 +36:25:09.6 -- not a known variable star
22:04:39.48 +41:55:44.1 -- not a known variable star
22:04:39.71 +37:04:27.3 -- not a known variable star
22:04:41.21 +40:20:51.2 -- a known variable star
22:04:43.21 +42:01:06.8 -- not a known variable star
22:04:44.36 +37:33:00.6 -- not a known variable star
22:04:46.29 +42:08:02.1 -- not a known variable star
22:04:51.38 +36:57:57.2 -- a known variable star
22:04:54.69 +35:49:32.1 -- not a known variable star
22:04:59.77 +39:57:17.5 -- a known variable star
22:05:09.75 +37:59:07.1 -- not a known variable star
22:05:27.15 +41:32:30.4 -- not a known variable star
22:05:27.65 +42:00:52.5 -- not a known variable star
22:05:32.49 +38:58:33.0 -- a known variable star
22:05:37.45 +38:57:41.0 -- not a known variable star
22:05:37.91 +35:36:47.0 -- not a known variable star
22:05:39.89 +34:53:38.5 -- a known variable star
22:05:42.70 +35:53:01.6 -- not a known variable star
22:05:48.96 +40:22:58.1 -- not a known variable star
22:05:53.67 +41:23:38.0 -- not a known variable star
22:05:58.50 +41:55:51.3 -- not a known variable star
22:06:02.05 +40:00:16.4 -- not a known variable star
22:06:02.53 +38:59:35.1 -- not a known variable star
22:06:05.56 +41:38:13.1 -- not a known variable star
22:06:09.41 +39:56:12.0 -- not a known variable star
22:06:12.37 +39:36:03.7 -- not a known variable star
22:06:13.56 +41:38:26.9 -- not a known variable star
22:06:23.77 +41:39:59.2 -- not a known variable star
22:06:24.16 +38:41:47.2 -- not a known variable star
22:06:27.14 +39:09:53.4 -- not a known variable star
22:06:28.76 +39:03:18.4 -- not a known variable star
22:06:29.11 +39:32:46.8 -- not a known variable star
22:06:30.62 +34:18:24.6 -- not a known variable star
22:06:31.92 +34:33:33.0 -- not a known variable star
22:06:37.68 +41:44:03.3 -- not a known variable star
22:06:38.72 +41:43:51.1 -- not a known variable star
22:06:41.13 +40:11:40.3 -- not a known variable star
22:06:42.48 +40:57:13.5 -- not a known variable star
22:06:53.62 +39:49:46.3 -- not a known variable star
22:06:56.78 +36:48:40.3 -- a known variable star
22:07:02.72 +41:57:30.8 -- not a known variable star
22:07:10.96 +38:37:34.4 -- not a known variable star
22:07:12.31 +41:10:46.1 -- a known variable star
22:07:18.00 +39:07:48.0 -- a known variable star
22:07:22.71 +40:35:19.9 -- not a known variable star
22:07:23.06 +41:08:43.2 -- not a known variable star
22:07:31.14 +39:46:41.6 -- not a known variable star
22:07:35.18 +41:27:44.3 -- not a known variable star
22:07:43.41 +37:37:06.0 -- not a known variable star
22:07:48.92 +34:48:03.5 -- not a known variable star
22:07:52.46 +41:59:46.9 -- not a known variable star
22:07:53.03 +37:40:43.6 -- not a known variable star
22:08:01.57 +35:58:26.1 -- not a known variable star
22:08:02.15 +37:33:32.4 -- not a known variable star
22:08:05.92 +41:53:33.1 -- a known variable star
22:08:10.70 +39:02:02.5 -- a known variable star
22:08:12.38 +39:44:12.0 -- not a known variable star
22:08:21.44 +34:16:43.6 -- not a known variable star
22:08:28.16 +41:17:32.5 -- not a known variable star
22:08:28.75 +34:30:21.8 -- not a known variable star
22:08:34.63 +37:33:22.7 -- not a known variable star
22:08:43.68 +41:30:45.0 -- not a known variable star
22:08:49.92 +40:21:08.2 -- not a known variable star
22:08:55.68 +38:16:52.9 -- not a known variable star
22:08:56.95 +41:29:27.8 -- not a known variable star
22:08:57.22 +36:50:52.7 -- not a known variable star
22:08:58.89 +42:02:06.8 -- not a known variable star
22:09:10.00 +41:58:24.6 -- not a known variable star
22:09:10.52 +33:47:36.6 -- not a known variable star
22:09:11.66 +36:46:05.4 -- not a known variable star
22:09:13.59 +39:15:46.5 -- not a known variable star
22:09:18.89 +39:53:05.4 -- a known variable star
22:09:33.65 +41:54:58.8 -- not a known variable star
22:09:46.32 +41:39:59.1 -- not a known variable star
22:09:51.75 +41:55:24.7 -- not a known variable star
22:09:55.37 +40:48:12.0 -- not a known variable star
22:09:59.93 +38:20:08.0 -- not a known variable star
22:10:02.92 +36:44:11.9 -- not a known variable star
22:10:06.42 +35:55:00.5 -- not a known variable star
22:10:14.91 +41:02:14.0 -- not a known variable star
22:10:15.85 +41:34:00.4 -- not a known variable star
22:10:20.20 +38:44:20.8 -- a known variable star
22:10:20.81 +41:33:09.1 -- not a known variable star
22:10:32.03 +41:45:05.9 -- a known variable star
22:10:36.56 +39:03:13.4 -- not a known variable star
22:10:43.52 +41:09:26.3 -- not a known variable star
22:10:57.04 +37:02:43.5 -- not a known variable star
22:11:02.23 +38:11:05.6 -- not a known variable star
22:11:07.15 +41:20:25.4 -- not a known variable star
22:11:07.90 +41:18:47.3 -- a known variable star
22:11:12.81 +41:39:57.6 -- not a known variable star
22:11:31.18 +40:27:17.9 -- not a known variable star
22:11:35.58 +41:59:08.7 -- not a known variable star
22:11:43.30 +42:07:49.5 -- not a known variable star
22:11:45.13 +41:45:55.6 -- not a known variable star
22:11:50.18 +39:03:26.3 -- not a known variable star
22:11:52.00 +42:03:53.3 -- a known variable star
22:11:52.66 +40:52:48.1 -- not a known variable star
22:12:02.15 +41:01:53.3 -- a known variable star
22:12:04.92 +39:17:50.0 -- not a known variable star
22:12:09.67 +41:33:21.3 -- not a known variable star
22:12:24.03 +40:35:38.7 -- not a known variable star
Found 549 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
639 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 639 (excluding asteroids and hot pixels, 549 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461185.84774850 -observatory V36
04:59:58.60 +24:28:41.6 Mercury (-1.2mag)
06:31:31.82 +25:01:11.4 Venus (-3.9mag)
02:09:39.49 +12:20:54.4 Mars (1.3mag)
07:37:20.56 +21:57:52.6 Jupiter (-1.9mag)
00:45:00.95 +02:24:14.9 Saturn (0.9mag)
03:56:51.96 +20:15:42.6 Uranus (5.8mag)
00:15:09.62 +00:11:09.5 Neptune (7.8mag)
20:33:57.93 -22:59:48.3 Pluto (14.5mag)
11:40:27.62 -00:47:22.3 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 363 May 25 05:50 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461185.84774850:
07:37:27.86 +21:57:34.0 Io (5.9mag)
07:37:27.89 +21:57:34.5 Europa (6.1mag)
07:37:04.96 +21:58:37.2 Ganymede (5.5mag)
07:37:06.46 +21:58:23.8 Callisto (6.7mag)
07:38:28.78 +21:34:17.2 Himalia (15.5mag)
07:37:17.96 +21:58:00.6 Thebe (16.5mag)
07:38:48.08 +21:55:54.5 Elara (17.5mag)
07:38:45.46 +22:17:04.8 Pasiphae (17.7mag)
07:44:29.61 +21:58:39.1 Carme (18.8mag)
00:44:59.34 +02:23:58.5 Titan (8.7mag)
00:44:59.61 +02:24:30.0 Rhea (10.0mag)
00:45:22.02 +02:24:12.5 Iapetus (11.4mag)
00:45:16.29 +02:24:11.3 Hyperion (14.7mag)
00:45:59.53 +02:28:08.8 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 05:50 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461185.84774850:
17:15:52.36 -33:12:09.1 JWST
19:56:54.67 -02:39:41.1 Chandra
20:13:50.65 +26:07:26.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 05:50 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461185.84774850 -observatory V36
13:21:29.27 -27:08:45.4 14.4mag D/1884 O1 (Barnard)
06:35:54.72 +30:41:36.1 15.7mag D/1886 K1 (Brooks)
15:27:03.60 +01:18:51.2 14.6mag D/1895 Q1 (Swift)
05:26:50.32 +24:37:05.9 17.2mag D/1918 W1 (Schorr)
09:25:28.97 +15:18:09.6 17.9mag P/2009 WX51 (Catalina)
18:51:23.44 -31:35:29.9 13.7mag P/2010 H2 (Vales)
05:40:05.69 -68:17:05.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:03.72 +31:47:55.1 17.4mag C/2017 K2 (PANSTARRS)
17:20:10.63 +14:29:15.4 17.7mag C/2021 G2 (ATLAS)
23:14:36.50 +31:00:34.8 17.2mag C/2022 E2 (ATLAS)
05:16:58.79 +26:50:51.3 16.4mag C/2022 N2 (PANSTARRS)
09:20:26.61 +31:30:59.2 16.5mag C/2022 QE78 (ATLAS)
08:43:37.90 +03:09:59.6 17.6mag C/2022 R6 (PANSTARRS)
18:36:51.29 +21:10:10.8 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:47.77 -11:02:34.2 17.5mag P/2023 B1 (PANSTARRS)
22:16:09.49 +65:36:14.5 17.7mag C/2023 H5 (Lemmon)
18:18:56.36 -05:28:15.6 13.7mag C/2023 R1 (PANSTARRS)
13:42:49.59 +85:58:01.6 17.9mag C/2023 X2 (Lemmon)
06:52:25.40 +63:54:27.5 17.6mag C/2024 A1 (ATLAS)
06:25:32.27 +26:22:50.1 13.1mag C/2024 E1 (Wierzchos)
15:48:34.74 +12:06:46.8 17.3mag C/2024 G6 (ATLAS)
20:20:06.61 +26:55:01.2 14.1mag C/2024 J3 (ATLAS)
04:04:09.01 -17:17:30.3 16.1mag C/2024 T5 (ATLAS)
05:52:52.30 +36:58:06.9 17.9mag C/2025 J1 (Borisov)
11:46:43.70 +53:21:30.0 16.9mag C/2025 L1 (ATLAS)
06:23:14.16 -10:07:39.8 12.5mag C/2025 R3 (PANSTARRS)
12:41:05.61 +04:36:13.2 17.2mag C/2025 Y1 (ATLAS)
01:34:38.70 +42:18:30.7 15.7mag C/2026 B2 (Sun-Gao)
11:10:31.03 -09:22:16.6 16.2mag A/2026 E1
19:58:06.62 -08:07:20.6 9.5mag 10P/Tempel
14:19:07.99 -02:27:08.8 17.6mag 24P/Schaumasse
10:59:37.47 -00:51:51.1 15.9mag 29P/Schwassmann-Wachmann
10:50:46.18 -02:34:20.3 17.7mag 43P/Wolf-Harrington
02:50:09.46 +23:42:56.3 17.6mag 47P/Ashbrook-Jackson
08:30:28.45 +27:35:26.9 16.9mag 63P/Wild
00:14:03.60 -07:23:27.5 15.7mag 65P/Gunn
05:59:00.18 +31:32:39.1 16.5mag 76P/West-Kohoutek-Ikemura
02:35:59.05 +15:15:46.6 13.9mag 78P/Gehrels
00:49:10.18 +01:36:46.2 15.3mag 88P/Howell
04:10:06.34 +28:49:56.9 15.1mag 93P/Lovas
02:05:13.51 +25:11:48.7 18.0mag 114P/Wiseman-Skiff
06:18:04.43 +33:19:49.9 15.7mag 123P/West-Hartley
09:26:33.79 +20:38:01.7 16.4mag 124P/Mrkos
03:36:14.16 +18:13:18.7 16.4mag 128P/Shoemaker-Holt
04:05:54.20 +18:17:30.9 17.7mag 131P/Mueller
04:54:38.66 +19:40:02.1 12.9mag 141P/Machholz
04:57:20.15 +16:15:20.2 12.8mag 141P-A/Machholz
03:42:05.51 +13:31:02.8 10.6mag 141P-D/Machholz
02:47:34.59 -26:47:19.6 17.3mag 161P/Hartley-IRAS
02:57:18.37 +17:51:13.2 14.9mag 162P/SidingSpring
19:34:27.41 -01:54:31.7 17.6mag 169P/NEAT
17:02:59.15 -09:25:52.1 16.2mag 235P/LINEAR
07:03:07.61 +35:52:35.5 17.3mag 240P/NEAT
23:56:24.62 -08:05:40.2 16.8mag 260P/McNaught
03:27:53.32 +29:44:49.2 17.7mag 295P/LINEAR
21:56:49.28 -28:33:17.8 17.7mag 320P/McNaught
15:22:11.73 +08:21:51.9 17.4mag 391P/Kowalski
07:56:36.98 +21:03:15.1 17.8mag 450P/LONEOS
06:37:24.20 +42:38:31.6 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 05:50 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 25 05:50 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 25 05:50 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:48:01.526 -06:28:12.25 AT 2026mxj 2026-05-12.44 20.712
15:26:54.440 -08:30:53.42 AT 2026mxi 2026-05-11.31 20.7559
18:52:51.594 -18:48:35.64 AT 2026mxh 2026-05-14.41 19.2802
12:23:56.695 +21:12:04.15 SN 2026mxg 2026-05-15.26 20.5476
16:26:51.090 +23:30:02.07 AT 2026mxf 2026-05-09.79 20.19
12:32:29.870 +24:17:28.39 AT 2026mxe 2026-05-07.78 20.84
18:52:28.230 +41:35:58.05 AT 2026mxd 2026-05-06.77 20.29
16:01:49.510 +16:19:54.29 AT 2026mxc 2026-05-03.86 20.43
13:07:34.620 +48:36:49.59 AT 2026mxb 2026-04-28.84 21.35
12:41:13.920 +28:45:38.69 AT 2026mxa 2026-04-28.86 20.83
17:59:59.500 +26:37:11.25 AT 2026mwz 2026-04-27.89 21.34
12:28:50.550 +41:12:21.53 AT 2026mwy 2026-04-24.82 20.86
14:02:54.920 +52:50:36.73 AT 2026mwx 2026-04-19.86 21.51
12:33:02.940 +24:34:37.91 AT 2026mww 2026-04-15.87 21.01
16:40:46.740 +26:54:33.05 AT 2026mwv 2026-04-12.76 21.07
13:03:52.940 +23:49:42.82 AT 2026mwu 2026-04-03.87 20.84
17:45:23.200 +33:15:24.68 AT 2026mwt 2026-03-30.83 20.98
13:11:30.630 +21:00:44.67 AT 2026mws 2026-03-23.71 21.69
12:21:33.740 +27:53:15.15 AT 2026mwr 2026-03-23.70 21
14:26:34.570 +01:19:55.58 AT 2026mwq 2026-05-11.69 22.6
-rw-r--r-- 1 apache apache 30K May 25 05:50 tns_transients_list.txt
