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-Q1b1x1_033929_TTUQ1b1x1_3226133_znNLp9oG
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 25.3473 2461185.8473 12.25 21:40:23.65 +39:00:27.7
87.15585 -10.24671 galactic Cyg Second-epoch detections are separated by 2.1" and 6.6 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 | 21:40:23.65 +39:00:27.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:23.65 +39:00:27.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:23.65 +39:00:27.7: 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
target,2461185.8473,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.39 21:35:50.35 +40:48:09.1
87.72688 -8.33184 galactic Cyg Second-epoch detections are separated by 3.1" and 6.3 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 J323.9697+40.7953 | 21:35:50.35 +40:48:09.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K4 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:50.35 +40:48:09.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:50.35 +40:48:09.1: 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 J323.9697+40.7953,2461185.8473,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.9697+40.7953 20260525.3473 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 25.3473 2461185.8473 12.13 21:56:08.18 +40:50:21.0
90.69988 -10.81177 galactic Cyg Second-epoch detections are separated by 2.9" and 6.6 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 | 21:56:08.18 +40:50:21.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.804+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:08.18 +40:50:21.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:08.18 +40:50:21.0: 14.00 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.24 21:43:42.41 +42:34:57.7
90.03188 -7.98606 galactic Cyg Second-epoch detections are separated by 2.3" and 6.5 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 | 21:43:42.41 +42:34:57.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:42.41 +42:34:57.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:42.41 +42:34:57.7: 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
target,2461185.8473,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.19 22:06:54.81 +41:38:24.7
92.83188 -11.41953 galactic Lac Second-epoch detections are separated by 2.4" and 6.7 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 | 22:06:54.81 +41:38:24.7 (user input) | T | P | (position from user input) J-Ks=0.698+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:54.81 +41:38:24.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:54.81 +41:38:24.7: 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.15 21:45:30.06 +40:39:22.2
89.00996 -9.66065 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 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 | 21:45:30.06 +40:39:22.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:30.06 +40:39:22.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:30.06 +40:39:22.2: 14.54 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.54 +/- 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,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.22 21:40:19.25 +38:45:41.7
86.97750 -10.41989 galactic Cyg Second-epoch detections are separated by 0.6" and 6.8 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 | 21:40:19.25 +38:45:41.7 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:19.25 +38:45:41.7: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:19.25 +38:45:41.7: 13.96 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461185.8473,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.08 21:32:26.27 +37:28:42.2
84.93497 -10.30540 galactic Cyg Second-epoch detections are separated by 4.7" and 6.6 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 | 21:32:26.27 +37:28:42.2 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:26.27 +37:28:42.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:26.27 +37:28:42.2: 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,2461185.8473,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.29 21:32:28.08 +38:05:43.0
85.37162 -9.86294 galactic Cyg Second-epoch detections are separated by 0.7" and 7.0 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 1952269863916728320 | 21:32:31.69 +38:05:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.480+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:28.08 +38:05:43.0: 12.84 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:28.08 +38:05:43.0: 14.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 1952269863916728320,2461185.8473,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1952269863916728320 20260525.3473 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 25.3473 2461185.8473 12.14 21:14:40.71 +37:16:07.6
82.26769 -7.94822 galactic Cyg Second-epoch detections are separated by 4.2" and 7.4 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 J318.6705+37.2688 | 21:14:40.71 +37:16:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:40.71 +37:16:07.6: 12.57 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:40.71 +37:16:07.6: 14.22 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 J318.6705+37.2688,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.6705+37.2688 20260525.3473 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 25.3473 2461185.8473 12.14 21:29:38.32 +39:05:20.9
85.66390 -8.76285 galactic Cyg Second-epoch detections are separated by 0.7" and 6.9 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 | 21:29:38.32 +39:05:20.9 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.055 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:38.32 +39:05:20.9: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:38.32 +39:05:20.9: 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
target,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.11 21:41:18.31 +41:17:54.2
88.83584 -8.65565 galactic Cyg Second-epoch detections are separated by 4.3" and 6.9 pix
The object was found in VSX15" Gaia DR3 1966543723867908736
Type: S
# Max. Min./Amp. JD0 Period
16.090 G 16.980 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:18.31 +41:17:54.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:18.31 +41:17:54.2: 14.11 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 1966543723867908736,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1966543723867908736 20260525.3473 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 25.3473 2461185.8473 12.13 21:40:47.73 +38:06:20.2
86.60037 -10.96908 galactic Cyg Second-epoch detections are separated by 2.0" and 7.2 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 | ASASSN-V J214046.49+380540.0 | 21:40:46.49 +38:05:40.0 (Gaia DR3) | EA (local) | 2459053.86200 (local) | Gaia3var=VARIABLE SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:47.73 +38:06:20.2: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:47.73 +38:06:20.2: 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
ASASSN-V J214046.49+380540.0,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J214046.49+380540.0 20260525.3473 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 25.3473 2461185.8473 11.98 21:19:52.54 +38:04:01.1
83.56810 -8.14020 galactic Cyg Second-epoch detections are separated by 4.4" and 7.0 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 J319.9781+38.0690 | 21:19:52.54 +38:04:01.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:52.54 +38:04:01.1: 12.99 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:52.54 +38:04:01.1: 14.02 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 J319.9781+38.0690,2461185.8473,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.9781+38.0690 20260525.3473 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 25.3473 2461185.8473 12.11 21:15:31.73 +38:37:42.4
83.38100 -7.13661 galactic Cyg Second-epoch detections are separated by 3.4" and 6.9 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 | 21:15:31.73 +38:37:42.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:31.73 +38:37:42.4: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:31.73 +38:37:42.4: 14.19 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.98 21:53:19.50 +34:36:59.1
86.19096 -15.25543 galactic Peg Second-epoch detections are separated by 3.9" and 7.6 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 | 21:53:19.50 +34:36:59.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:19.50 +34:36:59.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:19.50 +34:36:59.1: 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
target,2461185.8473,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.09 21:28:14.41 +42:51:46.0
88.11167 -5.86168 galactic Cyg Second-epoch detections are separated by 4.6" and 6.5 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 J322.0695+42.8626 | 21:28:14.41 +42:51:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:14.41 +42:51:46.0: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:14.41 +42:51:46.0: 13.93 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 J322.0695+42.8626,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.0695+42.8626 20260525.3473 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 25.3473 2461185.8473 11.95 21:24:56.62 +36:58:07.4
83.49019 -9.62682 galactic Cyg Second-epoch detections are separated by 0.9" and 6.8 pix
The object was found in VSX20" Gaia DR3 1963741446687127808
Type: ROT
# Max. Min./Amp. JD0 Period
14.320 G 14.370 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:56.62 +36:58:07.4: 13.14 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:56.62 +36:58:07.4: 13.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 1963741446687127808,2461185.8473,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963741446687127808 20260525.3473 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 25.3473 2461185.8473 11.85 22:08:04.65 +35:52:50.9
89.45185 -16.15807 galactic Lac Second-epoch detections are separated by 3.1" and 7.7 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 | 22:08:04.65 +35:52:50.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:04.65 +35:52:50.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:04.65 +35:52:50.9: 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,2461185.8473,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.27 21:21:23.82 +41:56:52.4
86.56189 -5.62748 galactic Cyg Second-epoch detections are separated by 2.9" and 6.6 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 J320.3524+41.9600 | 21:21:23.82 +41:56:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.844+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:23.82 +41:56:52.4: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:23.82 +41:56:52.4: 14.64 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.64 +/- 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 J320.3524+41.9600,2461185.8473,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.3524+41.9600 20260525.3473 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 25.3473 2461185.8473 12.03 21:35:24.40 +36:45:52.6
84.87274 -11.23058 galactic Cyg Second-epoch detections are separated by 2.6" and 6.8 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 | 21:35:24.40 +36:45:52.6 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.050 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:24.40 +36:45:52.6: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:24.40 +36:45:52.6: 14.39 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.39 +/- 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,2461185.8473,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.98 22:09:56.43 +39:05:39.8
91.75327 -13.80818 galactic Lac Second-epoch detections are separated by 1.4" and 6.9 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 | 22:09:56.43 +39:05:39.8 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:56.43 +39:05:39.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:56.43 +39:05:39.8: 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,2461185.8473,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.01 21:16:29.78 +36:27:23.2
81.92263 -8.77013 galactic Cyg Second-epoch detections are separated by 3.4" and 6.8 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 J319.1355+36.4547 | 21:16:29.78 +36:27:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:29.78 +36:27:23.2: 12.11 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:29.78 +36:27:23.2: 14.14 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 J319.1355+36.4547,2461185.8473,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1355+36.4547 20260525.3473 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 25.3473 2461185.8473 11.97 21:14:58.71 +40:12:43.0
84.46324 -5.96922 galactic Cyg Second-epoch detections are separated by 2.4" and 6.5 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 | 21:14:58.71 +40:12:43.0 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:58.71 +40:12:43.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:58.71 +40:12:43.0: 14.08 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461185.8473,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.06 21:30:49.11 +38:57:23.2
85.73800 -9.01732 galactic Cyg Second-epoch detections are separated by 1.7" and 6.8 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 J322.7033+38.9578 | 21:30:49.11 +38:57:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:49.11 +38:57:23.2: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:49.11 +38:57:23.2: 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 J322.7033+38.9578,2461185.8473,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.7033+38.9578 20260525.3473 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 25.3473 2461185.8473 11.92 21:21:41.70 +36:14:58.9
82.50658 -9.66798 galactic Cyg Second-epoch detections are separated by 1.7" and 7.2 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 J320.4313+36.2480 | 21:21:41.70 +36:14:58.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:41.70 +36:14:58.9: 13.25 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:41.70 +36:14:58.9: 14.05 +/- 0.11 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
ATO J320.4313+36.2480,2461185.8473,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.4313+36.2480 20260525.3473 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3473 2461185.8473 11.86 21:46:34.06 +35:50:36.5
85.94118 -13.42484 galactic Cyg Second-epoch detections are separated by 5.7" and 7.5 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 | 21:46:34.06 +35:50:36.5 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:34.06 +35:50:36.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:34.06 +35:50:36.5: 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
target,2461185.8473,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.96 22:24:04.86 +41:24:51.1
95.39497 -13.44650 galactic Lac Second-epoch detections are separated by 4.6" and 7.7 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 | 22:24:04.86 +41:24:51.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:04.86 +41:24:51.1: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:04.86 +41:24:51.1: 14.61 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.61 +/- 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,2461185.8473,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.88 21:11:00.67 +40:05:05.5
83.84871 -5.50335 galactic Cyg Second-epoch detections are separated by 3.6" and 7.1 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 J317.7549+40.0799 | 21:11:00.67 +40:05:05.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.063+/-0.024 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:00.67 +40:05:05.5: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:00.67 +40:05:05.5: 13.87 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 J317.7549+40.0799,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.7549+40.0799 20260525.3473 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 25.3473 2461185.8473 11.91 21:28:00.13 +36:42:32.1
83.74523 -10.24234 galactic Cyg Second-epoch detections are separated by 3.7" and 7.3 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 J321.9994+36.7025 | 21:28:00.13 +36:42:32.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:00.13 +36:42:32.1: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:00.13 +36:42:32.1: 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 J321.9994+36.7025,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.9994+36.7025 20260525.3473 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 25.3473 2461185.8473 11.78 21:37:34.51 +32:59:49.5
82.55427 -14.27688 galactic Cyg Second-epoch detections are separated by 1.1" and 7.2 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 | 21:37:34.51 +32:59:49.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:34.51 +32:59:49.5: 12.59 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:34.51 +32:59:49.5: 13.82 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461185.8473,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.81 21:10:29.46 +36:14:17.0
80.92856 -8.03336 galactic Cyg Second-epoch detections are separated by 1.2" and 6.9 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 J317.6229+36.2384 | 21:10:29.46 +36:14:17.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.161+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:29.46 +36:14:17.0: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:29.46 +36:14:17.0: 14.05 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 J317.6229+36.2384,2461185.8473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.6229+36.2384 20260525.3473 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 25.3473 2461185.8473 11.98 21:25:10.17 +35:57:12.1
82.79256 -10.37583 galactic Cyg Second-epoch detections are separated by 2.6" and 7.3 pix
The object was found in VSX14" Gaia DR3 1951579370616356608
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.790 G 15.840 G 0.552120000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:10.17 +35:57:12.1: 12.84 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:10.17 +35:57:12.1: 13.83 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 1951579370616356608,2461185.8473,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1951579370616356608 20260525.3473 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 25.3473 2461185.8473 11.93 21:19:42.35 +38:45:32.1
84.04536 -7.63383 galactic Cyg Second-epoch detections are separated by 2.9" and 7.2 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 J319.9282+38.7594 | 21:19:42.35 +38:45:32.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:42.35 +38:45:32.1: 12.63 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:42.35 +38:45:32.1: 13.76 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 J319.9282+38.7594,2461185.8473,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.9282+38.7594 20260525.3473 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 25.3473 2461185.8473 11.84 21:16:57.74 +37:32:50.0
82.78675 -8.08618 galactic Cyg Second-epoch detections are separated by 1.3" and 6.8 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 J319.2382+37.5501 | 21:16:57.74 +37:32:50.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.577+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:57.74 +37:32:50.0: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:57.74 +37:32:50.0: 14.14 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.14 +/- 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 J319.2382+37.5501,2461185.8473,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.2382+37.5501 20260525.3473 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 25.3473 2461185.8473 11.53 22:23:41.87 +34:37:03.3
91.38621 -19.05033 galactic Peg Second-epoch detections are separated by 4.3" and 7.0 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 | 22:23:41.87 +34:37:03.3 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:41.87 +34:37:03.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:41.87 +34:37:03.3: 14.60 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.60 +/- 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,2461185.8473,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.53CV 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 25.3473 2461185.8473 11.77 22:08:32.91 +35:58:48.5
89.59346 -16.13670 galactic Lac Second-epoch detections are separated by 0.2" and 7.3 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 | 22:08:32.91 +35:58:48.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:32.91 +35:58:48.5: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:32.91 +35:58:48.5: 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,2461185.8473,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.62 21:43:35.18 +37:22:30.0
86.52207 -11.88139 galactic Cyg Second-epoch detections are separated by 5.0" and 7.6 pix
The object was found in VSX10" V1984 Cyg
Type: M
# Max. Min./Amp. JD0 Period
14.000 B < 18.400 B 230.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:35.18 +37:22:30.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:35.18 +37:22:30.0: 14.48 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.48 +/- 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
V1984 Cyg,2461185.8473,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1984 Cyg 20260525.3473 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 25.3473 2461185.8473 11.82 21:27:27.41 +38:09:22.7
84.69614 -9.13416 galactic Cyg Second-epoch detections are separated by 1.8" and 6.7 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 J321.8640+38.1595 | 21:27:27.41 +38:09:22.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:27.41 +38:09:22.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:27.41 +38:09:22.7: 13.84 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 J321.8640+38.1595,2461185.8473,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.8640+38.1595 20260525.3473 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 25.3473 2461185.8473 11.86 21:16:43.12 +41:35:51.4
85.69767 -5.24884 galactic Cyg Second-epoch detections are separated by 5.2" and 6.4 pix
The object was found in VSX15" Gaia DR3 1968772910678647552
Type: VAR
# Max. Min./Amp. JD0 Period
18.310 G 18.410 G 0.014854600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:43.12 +41:35:51.4: 13.14 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:43.12 +41:35:51.4: 13.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 1968772910678647552,2461185.8473,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1968772910678647552 20260525.3473 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 25.3473 2461185.8473 11.79 22:15:54.18 +37:58:56.1
92.05496 -15.39277 galactic Lac Second-epoch detections are separated by 2.4" and 7.0 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 J333.9786+37.9704 | 22:15:54.18 +37:58:56.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:15:54.18 +37:58:56.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:15:54.18 +37:58:56.1: 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
ATO J333.9786+37.9704,2461185.8473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J333.9786+37.9704 20260525.3473 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 25.3473 2461185.8473 11.70 21:36:54.29 +40:36:45.6
87.74733 -8.60829 galactic Cyg Second-epoch detections are separated by 0.6" and 6.7 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 J324.2332+40.6116 | 21:36:54.29 +40:36:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:54.29 +40:36:45.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:54.29 +40:36:45.6: 13.98 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 J324.2332+40.6116,2461185.8473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.2332+40.6116 20260525.3473 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 25.3473 2461185.8473 11.62 22:24:00.62 +40:01:13.8
94.59316 -14.60298 galactic Lac Second-epoch detections are separated by 4.8" and 8.0 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 1908959413700466176 | 22:24:02.82 +40:01:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:00.62 +40:01:13.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:00.62 +40:01:13.8: 13.87 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 1908959413700466176,2461185.8473,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1908959413700466176 20260525.3473 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 25.3473 2461185.8473 11.55 21:24:53.95 +33:31:57.4
80.99788 -12.03841 galactic Cyg Second-epoch detections are separated by 2.2" and 7.0 pix
The object was found in VSX17" Gaia DR3 1854967998302861312
Type: ROT
# Max. Min./Amp. JD0 Period
15.470 G 15.530 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:53.95 +33:31:57.4: 12.04 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:53.95 +33:31:57.4: 14.15 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.92 +/- 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
Gaia DR3 1854967998302861312,2461185.8473,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1854967998302861312 20260525.3473 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 25.3473 2461185.8473 11.69 21:18:37.33 +33:54:03.0
80.34346 -10.84345 galactic Cyg Second-epoch detections are separated by 2.0" and 6.8 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 | 21:18:37.33 +33:54:03.0 (user input) | T | P | (position from user input) J-Ks=0.817+/-0.029 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:37.33 +33:54:03.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:37.33 +33:54:03.0: 14.03 +/- 0.13 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,2461185.8473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.70 21:11:57.97 +36:45:24.9
81.51694 -7.90083 galactic Cyg Second-epoch detections are separated by 0.9" and 6.9 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 J317.9888+36.7572 | 21:11:57.97 +36:45:24.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:57.97 +36:45:24.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:57.97 +36:45:24.9: 13.96 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 J317.9888+36.7572,2461185.8473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.9888+36.7572 20260525.3473 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 25.3473 2461185.8473 11.46 21:50:49.89 +33:01:37.9
84.70699 -16.12301 galactic Peg Second-epoch detections are separated by 3.0" and 7.7 pix
The object was found in VSX16" Gaia DR3 1946544397630700928
Type: ROT
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 20.016000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:49.89 +33:01:37.9: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:49.89 +33:01:37.9: 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
Gaia DR3 1946544397630700928,2461185.8473,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1946544397630700928 20260525.3473 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 25.3473 2461185.8473 11.80 21:14:59.46 +34:09:50.9
80.01501 -10.11477 galactic Cyg Second-epoch detections are separated by 0.4" and 7.2 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 J318.7555+34.1575 | 21:14:59.46 +34:09:50.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.516+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:59.46 +34:09:50.9: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:59.46 +34:09:50.9: 13.90 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 J318.7555+34.1575,2461185.8473,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.7555+34.1575 20260525.3473 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 25.3473 2461185.8473 11.54 22:13:08.46 +40:02:52.1
92.84347 -13.40003 galactic Lac Second-epoch detections are separated by 2.1" and 6.8 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 | 22:13:08.46 +40:02:52.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.730+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:13:08.46 +40:02:52.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:13:08.46 +40:02:52.1: 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
target,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.65 21:17:19.92 +34:34:11.1
80.65125 -10.19001 galactic Cyg Second-epoch detections are separated by 6.7" and 7.0 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 | 21:17:19.92 +34:34:11.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:19.92 +34:34:11.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:19.92 +34:34:11.1: 13.71 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461185.8473,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.53 22:20:24.64 +41:35:26.1
94.90767 -12.91901 galactic Lac Second-epoch detections are separated by 5.7" and 7.0 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 | 22:20:24.64 +41:35:26.1 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:24.64 +41:35:26.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:24.64 +41:35:26.1: 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
target,2461185.8473,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.53CV 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 25.3473 2461185.8473 11.66 22:12:22.91 +41:42:04.4
93.71089 -11.97234 galactic Lac Second-epoch detections are separated by 1.2" and 7.2 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 | 22:12:22.91 +41:42:04.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:22.91 +41:42:04.4: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:22.91 +41:42:04.4: 13.62 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461185.8473,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.71 21:25:03.54 +33:29:46.4
80.99521 -12.08767 galactic Cyg Second-epoch detections are separated by 1.1" and 7.0 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 J321.2637+33.4988 | 21:25:03.54 +33:29:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:03.54 +33:29:46.4: 12.24 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:03.54 +33:29:46.4: 13.85 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 J321.2637+33.4988,2461185.8473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.2637+33.4988 20260525.3473 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 25.3473 2461185.8473 11.46 22:27:59.83 +41:57:08.5
96.32657 -13.39088 galactic Lac Second-epoch detections are separated by 0.9" and 7.5 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 J337.0073+41.9574 | 22:27:59.83 +41:57:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.645+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:59.83 +41:57:08.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:59.83 +41:57:08.5: 14.13 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 J337.0073+41.9574,2461185.8473,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J337.0073+41.9574 20260525.3473 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 25.3473 2461185.8473 11.54 22:26:53.22 +41:24:28.4
95.84544 -13.73825 galactic Lac Second-epoch detections are separated by 2.7" and 7.6 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 J336.7201+41.4086 | 22:26:53.22 +41:24:28.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:53.22 +41:24:28.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:53.22 +41:24:28.4: 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
ATO J336.7201+41.4086,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.7201+41.4086 20260525.3473 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 25.3473 2461185.8473 11.58 21:16:05.12 +35:26:56.5
81.12291 -9.40117 galactic Cyg Second-epoch detections are separated by 1.2" and 6.8 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 | 21:16:05.12 +35:26:56.5 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:05.12 +35:26:56.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:05.12 +35:26:56.5: 13.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461185.8473,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.58CV 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 25.3473 2461185.8473 11.53 21:26:27.74 +35:10:57.9
82.42621 -11.10618 galactic Cyg Second-epoch detections are separated by 3.9" and 7.6 pix
The object was found in VSX10" Gaia DR3 1951287553357722240
Type: RS
# Max. Min./Amp. JD0 Period
13.670 G 13.720 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:27.74 +35:10:57.9: 11.74 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:27.74 +35:10:57.9: 13.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 1951287553357722240,2461185.8473,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1951287553357722240 20260525.3473 11.53CV 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 25.3473 2461185.8473 11.54 21:57:39.23 +41:47:19.7
91.52959 -10.24822 galactic Lac Second-epoch detections are separated by 0.5" and 6.9 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 J329.4174+41.7911 | 21:57:39.23 +41:47:19.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.534+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:39.23 +41:47:19.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:39.23 +41:47:19.7: 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 J329.4174+41.7911,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 11.48 21:11:46.96 +36:20:55.9
81.18872 -8.15031 galactic Cyg Second-epoch detections are separated by 2.1" and 7.2 pix
The object was found in VSX13" Gaia DR3 1868485222459181440
Type: ROT
# Max. Min./Amp. JD0 Period
14.870 G 14.890 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:46.96 +36:20:55.9: 12.23 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:46.96 +36:20:55.9: 13.45 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 1868485222459181440,2461185.8473,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868485222459181440 20260525.3473 11.48CV 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 25.3473 2461185.8473 11.51 21:17:50.23 +39:58:39.7
84.67356 -6.52604 galactic Cyg Second-epoch detections are separated by 0.9" and 6.7 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 | 21:17:50.23 +39:58:39.7 (user input) | T | P | (position from user input) J-Ks=0.816+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:50.23 +39:58:39.7: 13.12 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:50.23 +39:58:39.7: 13.62 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.59 +/- 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,2461185.8473,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.51CV 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 25.3473 2461185.8473 11.59 21:22:48.69 +36:59:03.9
83.19744 -9.31345 galactic Cyg Second-epoch detections are separated by 0.7" and 6.8 pix
The object was found in VSX24" Gaia DR3 1963705231525248512
Type: ROT
# Max. Min./Amp. JD0 Period
12.850 G 12.880 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:48.69 +36:59:03.9: 11.76 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:48.69 +36:59:03.9: 13.53 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 1963705231525248512,2461185.8473,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963705231525248512 20260525.3473 11.59CV 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 25.3473 2461185.8473 11.45 21:40:35.21 +39:13:32.1
87.33220 -10.10981 galactic Cyg Second-epoch detections are separated by 1.8" and 6.8 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 | 21:40:35.21 +39:13:32.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.276+/-0.034 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:35.21 +39:13:32.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:35.21 +39:13:32.1: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 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,2461185.8473,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.45CV 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 25.3473 2461185.8473 11.39 21:14:41.88 +36:07:14.6
81.42398 -8.73638 galactic Cyg Second-epoch detections are separated by 5.3" and 6.6 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 | 21:14:41.88 +36:07:14.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:41.88 +36:07:14.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:41.88 +36:07:14.6: 13.54 +/- 0.08 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,2461185.8473,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.39CV 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 25.3473 2461185.8473 11.48 22:01:22.36 +40:55:08.1
91.54128 -11.36337 galactic Lac Second-epoch detections are separated by 0.1" and 7.0 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 J330.3389+40.9153 | 22:01:22.36 +40:55:08.1 (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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.36 +40:55:08.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:22.36 +40:55:08.1: 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 J330.3389+40.9153,2461185.8473,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 11.48CV 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 25.3473 2461185.8473 11.41 22:27:14.92 +42:09:27.2
96.31932 -13.14317 galactic Lac Second-epoch detections are separated by 2.3" and 7.5 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 | 22:27:14.92 +42:09:27.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:14.92 +42:09:27.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:14.92 +42:09:27.2: 13.77 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461185.8473,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.41CV 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 25.3473 2461185.8473 11.32 21:10:46.12 +35:46:39.9
80.62341 -8.38524 galactic Cyg Second-epoch detections are separated by 2.8" and 6.9 pix
The object was found in VSX18" Gaia DR3 1868060020697426048
Type: ROT
# Max. Min./Amp. JD0 Period
16.180 G 16.220 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:46.12 +35:46:39.9: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:46.12 +35:46:39.9: 13.46 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 1868060020697426048,2461185.8473,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868060020697426048 20260525.3473 11.32CV 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 25.3473 2461185.8473 11.40 21:09:31.20 +40:48:31.9
84.18946 -4.80372 galactic Cyg Second-epoch detections are separated by 2.9" and 6.9 pix
The object was found in VSX 9" Gaia DR3 1968570914078157056
Type: ROT
# Max. Min./Amp. JD0 Period
14.870 G 14.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:31.20 +40:48:31.9: 11.82 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:31.20 +40:48:31.9: 13.41 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 1968570914078157056,2461185.8473,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1968570914078157056 20260525.3473 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 25.3473 2461185.8473 11.39 21:17:13.96 +41:04:32.0
85.38748 -5.68071 galactic Cyg Second-epoch detections are separated by 2.3" and 7.0 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 | 21:17:13.96 +41:04:32.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:13.96 +41:04:32.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:13.96 +41:04:32.0: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.18 +/- 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,2461185.8473,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.39CV 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 25.3473 2461185.8473 11.16 21:13:58.21 +36:11:59.5
81.38106 -8.57500 galactic Cyg Second-epoch detections are separated by 6.0" and 7.4 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 J318.4962+36.1995 | 21:13:58.21 +36:11:59.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:58.21 +36:11:59.5: 12.95 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:58.21 +36:11:59.5: 13.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J318.4962+36.1995,2461185.8473,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.4962+36.1995 20260525.3473 11.16CV 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 25.3473 2461185.8473 11.32 21:12:24.72 +33:36:18.5
79.22902 -10.09998 galactic Cyg Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX 5" Gaia DR3 1866805031250947328
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.890 G 13.950 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:24.72 +33:36:18.5: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:24.72 +33:36:18.5: 13.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 1866805031250947328,2461185.8473,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1866805031250947328 20260525.3473 11.32CV 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 25.3473 2461185.8473 11.26 21:25:27.48 +37:40:36.4
84.07067 -9.19804 galactic Cyg Second-epoch detections are separated by 1.5" and 6.9 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 J321.3648+37.6768 | 21:25:27.48 +37:40:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.642+/- (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:27.48 +37:40:36.4: 12.44 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:27.48 +37:40:36.4: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 J321.3648+37.6768,2461185.8473,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.3648+37.6768 20260525.3473 11.26CV 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 25.3473 2461185.8473 11.24 22:23:06.22 +41:02:00.8
95.02162 -13.66312 galactic Lac Second-epoch detections are separated by 1.5" and 7.1 pix
The object was found in VSX 4" Gaia DR3 1957462135776539008
Type: ROT
# Max. Min./Amp. JD0 Period
14.030 G 14.050 G 0.560190000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:06.22 +41:02:00.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:06.22 +41:02:00.8: 13.62 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 1957462135776539008,2461185.8473,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957462135776539008 20260525.3473 11.24CV 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 25.3473 2461185.8473 11.20 22:20:44.67 +42:23:07.7
95.41484 -12.29393 galactic Lac Second-epoch detections are separated by 0.5" and 7.3 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 | 22:20:44.67 +42:23:07.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:44.67 +42:23:07.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:44.67 +42:23:07.7: 13.69 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461185.8473,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.20CV 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 25.3473 2461185.8473 11.29 21:20:10.14 +33:10:26.1
80.03284 -11.57793 galactic Cyg Second-epoch detections are separated by 2.7" and 6.9 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 | 21:20:10.14 +33:10:26.1 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:10.14 +33:10:26.1: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:10.14 +33:10:26.1: 13.48 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461185.8473,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.32 21:32:48.30 +39:29:39.6
86.39548 -8.89277 galactic Cyg Second-epoch detections are separated by 0.3" and 6.8 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 J323.2117+39.4959 | 21:32:48.30 +39:29:39.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:48.30 +39:29:39.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:48.30 +39:29:39.6: 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
ATO J323.2117+39.4959,2461185.8473,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.2117+39.4959 20260525.3473 11.32CV 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 25.3473 2461185.8473 11.24 21:21:29.43 +39:04:36.5
84.51958 -7.65940 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was found in VSX20" Gaia DR3 1965281965558099584
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.510 G 13.540 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:29.43 +39:04:36.5: 12.41 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:29.43 +39:04:36.5: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 1965281965558099584,2461185.8473,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1965281965558099584 20260525.3473 11.24CV 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 25.3473 2461185.8473 11.35 21:18:44.62 +36:41:41.9
82.41248 -8.93199 galactic Cyg Second-epoch detections are separated by 1.4" and 6.6 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 J319.6812+36.7067 | 21:18:44.62 +36:41:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.765+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:44.62 +36:41:41.9: 11.91 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:44.62 +36:41:41.9: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 J319.6812+36.7067,2461185.8473,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.6812+36.7067 20260525.3473 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 25.3473 2461185.8473 11.04 22:17:24.47 +38:35:02.3
92.66463 -15.07147 galactic Lac Second-epoch detections are separated by 1.1" and 7.2 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 | 22:17:24.47 +38:35:02.3 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:24.47 +38:35:02.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:24.47 +38:35:02.3: 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
target,2461185.8473,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.14 22:28:45.72 +41:44:04.0
96.33044 -13.65119 galactic Lac Second-epoch detections are separated by 1.2" and 7.7 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 J337.1815+41.7373 | 22:28:45.72 +41:44:04.0 (user input) | LPV (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.552+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:45.72 +41:44:04.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:45.72 +41:44:04.0: 14.12 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.12 +/- 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 J337.1815+41.7373,2461185.8473,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J337.1815+41.7373 20260525.3473 11.14CV 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 25.3473 2461185.8473 11.09 21:28:37.89 +35:33:42.3
83.01816 -11.14883 galactic Cyg Second-epoch detections are separated by 1.4" and 7.2 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 | 21:28:37.89 +35:33:42.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:37.89 +35:33:42.3: 11.98 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:37.89 +35:33:42.3: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 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,2461185.8473,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.09CV 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 25.3473 2461185.8473 11.14 21:48:46.98 +40:08:13.6
89.14851 -10.46144 galactic Cyg Second-epoch detections are separated by 1.7" and 7.0 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 J327.1964+40.1375 | 21:48:43.45 +40:08:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.035 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:46.98 +40:08:13.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:46.98 +40:08:13.6: 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
ATO J327.1964+40.1375,2461185.8473,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J327.1964+40.1375 20260525.3473 11.14CV 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 25.3473 2461185.8473 11.03 21:18:50.95 +34:56:39.7
81.14525 -10.15815 galactic Cyg Second-epoch detections are separated by 1.5" and 7.2 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 J319.7197+34.9474 | 21:18:52.73 +34:56:50.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:50.95 +34:56:39.7: 12.08 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:50.95 +34:56:39.7: 13.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 J319.7197+34.9474,2461185.8473,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.7197+34.9474 20260525.3473 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 25.3473 2461185.8473 11.08 21:19:25.52 +34:12:50.4
80.69118 -10.74814 galactic Cyg Second-epoch detections are separated by 3.0" and 6.8 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 J319.8488+34.2181 | 21:19:25.52 +34:12:50.4 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.317+/-0.029 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:25.52 +34:12:50.4: 12.28 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:25.52 +34:12:50.4: 13.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J319.8488+34.2181,2461185.8473,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.8488+34.2181 20260525.3473 11.08CV 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 25.3473 2461185.8473 11.09 21:11:10.88 +35:31:16.4
80.48912 -8.62018 galactic Cyg Second-epoch detections are separated by 1.0" and 6.9 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 J317.7891+35.5160 | 21:11:10.88 +35:31:16.4 (user input) | DBH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:10.88 +35:31:16.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:10.88 +35:31:16.4: 13.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 J317.7891+35.5160,2461185.8473,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.7891+35.5160 20260525.3473 11.09CV 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 25.3473 2461185.8473 11.00 22:28:39.45 +41:36:50.0
96.24716 -13.74267 galactic Lac Second-epoch detections are separated by 1.6" and 7.3 pix
The object was found in VSX21" Gaia DR3 1957556590697843456
Type: ROT
# Max. Min./Amp. JD0 Period
13.000 G 13.050 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:39.45 +41:36:50.0: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:39.45 +41:36:50.0: 13.49 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 1957556590697843456,2461185.8473,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957556590697843456 20260525.3473 11.00CV 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 25.3473 2461185.8473 11.01 21:12:41.04 +33:09:48.9
78.93659 -10.43968 galactic Cyg Second-epoch detections are separated by 1.0" and 7.4 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 1866777234222282496 | 21:12:39.04 +33:09:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:41.04 +33:09:48.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:41.04 +33:09:48.9: 12.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 1866777234222282496,2461185.8473,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1866777234222282496 20260525.3473 11.01CV 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 25.3473 2461185.8473 10.86 21:12:13.97 +35:19:19.8
80.48716 -8.91260 galactic Cyg Second-epoch detections are separated by 0.6" and 7.0 pix
The object was found in VSX16" Gaia DR3 1867282150581148032
Type: S
# Max. Min./Amp. JD0 Period
15.410 G 16.440 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:13.97 +35:19:19.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:13.97 +35:19:19.8: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 1867282150581148032,2461185.8473,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1867282150581148032 20260525.3473 10.86CV 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 25.3473 2461185.8473 10.88 21:17:20.41 +36:43:54.8
82.24270 -8.70323 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 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 J319.3393+36.7289 | 21:17:20.41 +36:43:54.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:20.41 +36:43:54.8: 11.68 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:20.41 +36:43:54.8: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 J319.3393+36.7289,2461185.8473,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3393+36.7289 20260525.3473 10.88CV 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 25.3473 2461185.8473 10.96 21:10:56.05 +35:44:07.0
80.61460 -8.43868 galactic Cyg Second-epoch detections are separated by 1.0" and 7.0 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 1868056928320957824 | 21:10:53.84 +35:44:28.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:56.05 +35:44:07.0: 12.05 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:56.05 +35:44:07.0: 13.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 1868056928320957824,2461185.8473,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868056928320957824 20260525.3473 10.96CV 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 25.3473 2461185.8473 10.83 21:20:25.11 +37:31:57.3
83.25654 -8.58971 galactic Cyg Second-epoch detections are separated by 0.7" and 7.0 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 J320.1010+37.5280 | 21:20:25.11 +37:31:57.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.648+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:25.11 +37:31:57.3: 11.59 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:25.11 +37:31:57.3: 12.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 J320.1010+37.5280,2461185.8473,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.1010+37.5280 20260525.3473 10.83CV 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 25.3473 2461185.8473 10.74 21:21:12.52 +36:20:37.3
82.50547 -9.53219 galactic Cyg Second-epoch detections are separated by 0.9" and 7.1 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 1963647331061827072 | 21:21:10.96 +36:20:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:12.52 +36:20:37.3: 11.48 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:12.52 +36:20:37.3: 12.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 1963647331061827072,2461185.8473,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963647331061827072 20260525.3473 10.74CV 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 25.3473 2461185.8473 10.61 21:53:17.43 +42:34:35.4
91.39193 -9.12778 galactic Cyg Second-epoch detections are separated by 3.0" and 6.5 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 1960662951568193792 | 21:53:17.23 +42:34:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.255+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:17.43 +42:34:35.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:17.43 +42:34:35.4: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 1960662951568193792,2461185.8473,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1960662951568193792 20260525.3473 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 25.3473 2461185.8473 10.63 21:18:26.61 +34:17:33.4
80.60681 -10.54698 galactic Cyg Second-epoch detections are separated by 2.5" and 6.9 pix
The object was found in VSX24" Gaia DR3 1855298951303505920
Type: ROT
# Max. Min./Amp. JD0 Period
14.690 G 14.720 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:26.61 +34:17:33.4: 11.56 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:26.61 +34:17:33.4: 12.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 1855298951303505920,2461185.8473,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1855298951303505920 20260525.3473 10.63CV 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 25.3473 2461185.8473 10.00 22:01:26.89 +38:07:17.1
89.78823 -13.57623 galactic Lac Second-epoch detections are separated by 1.6" and 6.8 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 | 22:01:26.89 +38:07:17.1 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.036 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:26.89 +38:07:17.1: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:26.89 +38:07:17.1: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 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,2461185.8473,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.00CV 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 25.3473 2461185.8473 9.76 21:13:16.12 +33:44:29.7
79.45352 -10.13923 galactic Cyg Second-epoch detections are separated by 0.9" and 7.2 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 1866900723121201408 | 21:13:14.46 +33:44:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:16.12 +33:44:29.7: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:16.12 +33:44:29.7: 11.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 1866900723121201408,2461185.8473,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1866900723121201408 20260525.3473 9.76CV 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 25.3473 2461185.8473 8.04 22:01:07.92 +39:15:18.7
90.45763 -12.64659 galactic Lac Second-epoch detections are separated by 1.1" and 6.9 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 | HIP 108695 | 22:01:06.72 +39:14:45.4 (Gaia DR3) | VAR (local) | 2.479670000000 (local) | Gaia3var=VARIABLE SpType: A0 1947IzKry...1...44S HD 209260 J-Ks=0.278+/-0.032 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:07.92 +39:15:18.7: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:07.92 +39:15:18.7: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.26 +/- 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
HIP 108695,2461185.8473,8.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HIP 108695 20260525.3473 8.04CV 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 25.3473 2461185.8473 9.09 21:31:14.91 +38:46:29.7
85.67210 -9.20633 galactic Cyg Second-epoch detections are separated by 0.2" and 6.8 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:14.91 +38:46:29.7: 12.58 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:14.91 +38:46:29.7: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461185.8473,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 9.09CV 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 25.3473 2461185.8473 9.37 22:29:53.35 +41:26:00.2
96.34902 -14.01826 galactic Lac Second-epoch detections are separated by 1.3" and 7.3 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 J337.4722+41.4238 | 22:29:53.38 +41:26:01.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.062+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:53.35 +41:26:00.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:53.35 +41:26:00.2: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 J337.4722+41.4238,2461185.8473,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J337.4722+41.4238 20260525.3473 9.37CV 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 25.3473 2461185.8473 10.00 21:15:17.47 +38:56:43.3
83.58054 -6.88491 galactic Cyg Second-epoch detections are separated by 1.2" and 6.6 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 J318.8439+38.9431 | 21:15:19.94 +38:56:57.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:17.47 +38:56:43.3: 11.74 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:17.47 +38:56:43.3: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 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 J318.8439+38.9431,2461185.8473,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.8439+38.9431 20260525.3473 10.00CV 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 25.3473 2461185.8473 10.29 22:09:13.49 +39:15:45.0
91.74135 -13.59055 galactic Lac Second-epoch detections are separated by 3.0" and 7.4 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:13.49 +39:15:45.0: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:13.49 +39:15:45.0: 12.35 +/- 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
Gaia DR3 1956289747146754688,2461185.8473,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 10.29CV 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 25.3473 2461185.8473 10.34 21:56:49.58 +42:13:05.3
91.67894 -9.81655 galactic Cyg Second-epoch detections are separated by 2.2" and 6.6 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 1960769363675990400 | 21:56:48.97 +42:13:32.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:49.58 +42:13:05.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:49.58 +42:13:05.3: 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 1960769363675990400,2461185.8473,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1960769363675990400 20260525.3473 10.34CV 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 25.3473 2461185.8473 10.19 21:27:28.52 +35:23:02.6
82.72025 -11.10957 galactic Cyg Second-epoch detections are separated by 1.6" and 6.9 pix
The object was found in VSX12" Gaia DR3 1951314727610397696
Type: E
# Max. Min./Amp. JD0 Period
18.840 G 19.590 G 0.297879000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:28.52 +35:23:02.6: 11.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:28.52 +35:23:02.6: 12.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 1951314727610397696,2461185.8473,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1951314727610397696 20260525.3473 10.19CV 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 25.3473 2461185.8473 10.49 21:30:37.79 +42:45:58.2
88.36331 -6.23420 galactic Cyg Second-epoch detections are separated by 0.3" and 6.6 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 1967421924425756544 | 21:30:39.89 +42:45:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.538+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:37.79 +42:45:58.2: 11.69 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:37.79 +42:45:58.2: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 1967421924425756544,2461185.8473,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1967421924425756544 20260525.3473 10.49CV 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 25.3473 2461185.8473 10.57 21:22:36.12 +35:35:48.8
82.16286 -10.25557 galactic Cyg Second-epoch detections are separated by 1.6" and 6.7 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 1855481710751928960 | 21:22:38.77 +35:35:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:36.12 +35:35:48.8: 10.92 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:36.12 +35:35:48.8: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.97 +/- 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 1855481710751928960,2461185.8473,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1855481710751928960 20260525.3473 10.57CV 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 25.3473 2461185.8473 10.56 21:21:47.77 +35:29:50.0
81.97405 -10.20788 galactic Cyg Second-epoch detections are separated by 1.7" and 6.9 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 1855474216027817600 | 21:21:45.57 +35:29:44.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:47.77 +35:29:50.0: 11.15 +/- 0.05 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:47.77 +35:29:50.0: 12.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 1855474216027817600,2461185.8473,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1855474216027817600 20260525.3473 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 25.3473 2461185.8473 10.63 21:26:25.16 +35:51:25.5
82.90519 -10.62293 galactic Cyg Second-epoch detections are separated by 2.1" and 6.8 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 J321.6060+35.8609 | 21:26:25.16 +35:51:25.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.349+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:25.16 +35:51:25.5: 11.45 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:25.16 +35:51:25.5: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 J321.6060+35.8609,2461185.8473,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.6060+35.8609 20260525.3473 10.63CV 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 25.3473 2461185.8473 10.69 21:26:53.16 +37:31:50.2
84.16992 -9.50098 galactic Cyg Second-epoch detections are separated by 0.9" and 6.8 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 J321.7099+37.5254 | 21:26:53.16 +37:31:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:53.16 +37:31:50.2: 11.99 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:53.16 +37:31:50.2: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 J321.7099+37.5254,2461185.8473,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.7099+37.5254 20260525.3473 10.69CV 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 25.3473 2461185.8473 10.77 21:23:35.11 +38:21:41.0
84.29661 -8.45313 galactic Cyg Second-epoch detections are separated by 1.5" and 6.8 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 J320.8920+38.3544 | 21:23:35.11 +38:21:41.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.383+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:35.11 +38:21:41.0: 10.88 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:35.11 +38:21:41.0: 12.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.83 +/- 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
ATO J320.8920+38.3544,2461185.8473,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.8920+38.3544 20260525.3473 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 25.3473 2461185.8473 10.86 22:02:13.82 +41:47:07.6
92.21106 -10.77625 galactic Lac Second-epoch detections are separated by 0.7" and 7.0 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 J330.5515+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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:13.82 +41:47:07.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:13.82 +41:47:07.6: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 J330.5515+41.7805,2461185.8473,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 10.86CV 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 25.3473 2461185.8473 10.91 21:15:42.98 +33:53:35.1
79.91746 -10.40946 galactic Cyg Second-epoch detections are separated by 1.7" and 7.4 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 J318.9171+33.8998 | 21:15:42.98 +33:53:35.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:42.98 +33:53:35.1: 12.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:42.98 +33:53:35.1: 12.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 J318.9171+33.8998,2461185.8473,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.9171+33.8998 20260525.3473 10.91CV 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 25.3473 2461185.8473 10.78 22:26:35.03 +36:53:06.5
93.23150 -17.49646 galactic Lac Second-epoch detections are separated by 1.6" and 7.3 pix
The object was found in VSX 8" ASASSN-V J222635.68+365305.4
Type: SR
# Max. Min./Amp. JD0 Period
13.990 V 14.560 V 2458353.16060 106.909972800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:35.03 +36:53:06.5: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:35.03 +36:53:06.5: 13.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 J222635.68+365305.4,2461185.8473,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J222635.68+365305.4 20260525.3473 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 25.3473 2461185.8473 10.89 21:24:39.66 +36:58:46.5
83.45755 -9.57918 galactic Cyg Second-epoch detections are separated by 0.7" and 6.9 pix
The object was found in VSX20" Gaia DR3 1963742408760031616
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.410 G 14.440 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:39.66 +36:58:46.5: 11.58 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:39.66 +36:58:46.5: 13.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 1963742408760031616,2461185.8473,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963742408760031616 20260525.3473 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 25.3473 2461185.8473 10.95 21:19:37.43 +35:07:20.3
81.38725 -10.14972 galactic Cyg Second-epoch detections are separated by 1.4" and 6.8 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 J319.9059+35.1167 | 21:19:37.43 +35:07:20.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:37.43 +35:07:20.3: 11.56 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:37.43 +35:07:20.3: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 J319.9059+35.1167,2461185.8473,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.9059+35.1167 20260525.3473 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 25.3473 2461185.8473 10.94 22:26:44.89 +40:34:42.4
95.35981 -14.42147 galactic Lac Second-epoch detections are separated by 1.3" and 7.5 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 | 22:26:44.89 +40:34:42.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:44.89 +40:34:42.4: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:44.89 +40:34:42.4: 13.96 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461185.8473,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.94CV 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 25.3473 2461185.8473 11.07 21:14:38.40 +37:33:48.6
82.47917 -7.74079 galactic Cyg Second-epoch detections are separated by 1.6" and 6.6 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 1868691174732587776 | 21:14:40.87 +37:33:33.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: F0 (LAMOST DR5) J-Ks=0.320+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:38.40 +37:33:48.6: 11.46 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:38.40 +37:33:48.6: 13.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 1868691174732587776,2461185.8473,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868691174732587776 20260525.3473 11.07CV 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 25.3473 2461185.8473 11.02 21:42:06.01 +36:50:53.0
85.93711 -12.07637 galactic Cyg Second-epoch detections are separated by 1.2" and 7.1 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 J325.5190+36.8572 | 21:42:02.55 +36:51:12.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:06.01 +36:50:53.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:06.01 +36:50:53.0: 13.47 +/- 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
ATO J325.5190+36.8572,2461185.8473,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.5190+36.8572 20260525.3473 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 25.3473 2461185.8473 11.06 21:20:52.17 +38:17:39.5
83.87025 -8.12125 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 1964847898984320640 | 21:20:48.66 +38:17:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/- (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:52.17 +38:17:39.5: 11.97 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:52.17 +38:17:39.5: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 1964847898984320640,2461185.8473,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1964847898984320640 20260525.3473 11.06CV 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 25.3473 2461185.8473 11.09 21:25:56.52 +38:11:59.2
84.51241 -8.89419 galactic Cyg Second-epoch detections are separated by 1.0" and 6.7 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 1964423968521888896 | 21:25:54.24 +38:12:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:56.52 +38:11:59.2: 13.04 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:56.52 +38:11:59.2: 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
Gaia DR3 1964423968521888896,2461185.8473,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1964423968521888896 20260525.3473 11.09CV 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 25.3473 2461185.8473 11.18 21:29:08.03 +42:01:02.7
87.64226 -6.58561 galactic Cyg Second-epoch detections are separated by 3.5" and 6.2 pix
The object was found in VSX 3" Gaia DR3 1967190545946435712
Type: ROT
# Max. Min./Amp. JD0 Period
14.270 G 14.290 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:08.03 +42:01:02.7: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:08.03 +42:01:02.7: 13.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 1967190545946435712,2461185.8473,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1967190545946435712 20260525.3473 11.18CV 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 25.3473 2461185.8473 10.98 22:07:49.45 +33:25:38.3
87.84407 -18.07160 galactic Peg Second-epoch detections are separated by 1.0" and 7.5 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 J331.9469+33.4302 | 22:07:49.45 +33:25:38.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:49.45 +33:25:38.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:49.45 +33:25:38.3: 13.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 J331.9469+33.4302,2461185.8473,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.9469+33.4302 20260525.3473 10.98CV 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 25.3473 2461185.8473 11.20 21:14:44.84 +38:12:03.0
82.96183 -7.31926 galactic Cyg Second-epoch detections are separated by 0.7" and 6.7 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 J318.6921+38.2089 | 21:14:44.84 +38:12:03.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:44.84 +38:12:03.0: 12.76 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:44.84 +38:12:03.0: 13.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 J318.6921+38.2089,2461185.8473,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.6921+38.2089 20260525.3473 11.20CV 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 25.3473 2461185.8473 11.19 21:29:04.95 +40:27:04.6
86.54148 -7.70809 galactic Cyg Second-epoch detections are separated by 1.0" and 6.6 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 J322.2754+40.4518 | 21:29:04.95 +40:27:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:04.95 +40:27:04.6: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:04.95 +40:27:04.6: 13.56 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 J322.2754+40.4518,2461185.8473,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.2754+40.4518 20260525.3473 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 25.3473 2461185.8473 11.45 21:17:59.54 +42:35:34.7
86.58039 -4.72610 galactic Cyg Second-epoch detections are separated by 3.8" and 6.2 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 J319.4983+42.5994 | 21:17:58.03 +42:35:59.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.644+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:59.54 +42:35:34.7: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:59.54 +42:35:34.7: 13.59 +/- 0.09 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
ATO J319.4983+42.5994,2461185.8473,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.4983+42.5994 20260525.3473 11.45CV 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 25.3473 2461185.8473 11.28 21:26:11.09 +42:43:43.7
87.74578 -5.69559 galactic Cyg Second-epoch detections are separated by 1.9" and 6.9 pix
The object was found in VSX 2" Gaia DR3 1970467812154650624
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.870 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:11.09 +42:43:43.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:11.09 +42:43:43.7: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 1970467812154650624,2461185.8473,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1970467812154650624 20260525.3473 11.28CV 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 25.3473 2461185.8473 11.16 21:49:54.44 +34:54:43.5
85.83854 -14.57418 galactic Peg Second-epoch detections are separated by 1.1" and 7.2 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 | 21:49:54.44 +34:54:43.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:54.44 +34:54:43.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:54.44 +34:54:43.5: 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
target,2461185.8473,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.16CV 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 25.3473 2461185.8473 11.22 22:06:46.45 +39:39:05.9
91.59108 -12.99573 galactic Lac Second-epoch detections are separated by 0.9" and 7.3 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 | 22:06:46.45 +39:39:05.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.641+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:46.45 +39:39:05.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:46.45 +39:39:05.9: 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,2461185.8473,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.41 21:12:49.51 +41:23:27.4
85.04277 -4.86322 galactic Cyg Second-epoch detections are separated by 0.9" and 6.7 pix
The object was found in VSX 1" V1234 Cyg
Type: M:
# Max. Min./Amp. JD0 Period
16.500 B < 18.000 B 2442723.00000 222.000000000000 M7-M9
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:49.51 +41:23:27.4: 12.45 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:49.51 +41:23:27.4: 14.30 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.47 +/- 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
V1234 Cyg,2461185.8473,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1234 Cyg 20260525.3473 11.41CV 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 25.3473 2461185.8473 11.33 21:12:50.84 +36:08:07.8
81.17744 -8.45276 galactic Cyg Second-epoch detections are separated by 2.6" and 7.1 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 J318.2116+36.1294 | 21:12:48.44 +36:07:43.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:50.84 +36:08:07.8: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:50.84 +36:08:07.8: 13.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 J318.2116+36.1294,2461185.8473,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.2116+36.1294 20260525.3473 11.33CV 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 25.3473 2461185.8473 11.38 21:15:36.32 +36:55:35.8
82.14405 -8.31734 galactic Cyg Second-epoch detections are separated by 1.7" and 7.1 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 1868608603976207488 | 21:15:33.71 +36:55:23.5 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:36.32 +36:55:35.8: 12.44 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:36.32 +36:55:35.8: 13.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 1868608603976207488,2461185.8473,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868608603976207488 20260525.3473 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 25.3473 2461185.8473 11.30 21:42:46.31 +37:59:49.7
86.82168 -11.30965 galactic Cyg Second-epoch detections are separated by 1.9" and 6.9 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 J325.6883+38.0053 | 21:42:43.15 +38:00:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:46.31 +37:59:49.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:46.31 +37:59:49.7: 13.65 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 J325.6883+38.0053,2461185.8473,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.6883+38.0053 20260525.3473 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 25.3473 2461185.8473 11.12 22:20:30.94 +33:33:35.0
90.17261 -19.54137 galactic Peg Second-epoch detections are separated by 1.4" and 7.5 pix
The object was found in VSX 2" Gaia DR3 1905073086772697088
Type: ROT
# Max. Min./Amp. JD0 Period
13.480 G 13.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:30.94 +33:33:35.0: 13.01 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:30.94 +33:33:35.0: 14.30 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 1905073086772697088,2461185.8473,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1905073086772697088 20260525.3473 11.12CV 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 25.3473 2461185.8473 11.28 22:21:21.34 +41:17:35.6
94.88820 -13.26459 galactic Lac Second-epoch detections are separated by 2.1" and 7.3 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 J335.3499+41.2971 | 22:21:21.34 +41:17:35.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:21.34 +41:17:35.6: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:21.34 +41:17:35.6: 13.89 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 J335.3499+41.2971,2461185.8473,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.3499+41.2971 20260525.3473 11.28CV 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 25.3473 2461185.8473 11.21 22:09:21.19 +33:46:49.3
88.33591 -17.98633 galactic Peg Second-epoch detections are separated by 0.8" and 7.5 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 | 22:09:21.19 +33:46:49.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:21.19 +33:46:49.3: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:21.19 +33:46:49.3: 14.14 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461185.8473,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.39 21:15:25.79 +36:10:50.5
81.57050 -8.80311 galactic Cyg Second-epoch detections are separated by 2.8" and 7.4 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 J318.8553+36.1819 | 21:15:25.79 +36:10:50.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.448+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:25.79 +36:10:50.5: 12.90 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:25.79 +36:10:50.5: 13.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.23 +/- 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 J318.8553+36.1819,2461185.8473,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.8553+36.1819 20260525.3473 11.39CV 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 25.3473 2461185.8473 11.39 21:44:49.72 +36:56:53.9
86.42181 -12.36484 galactic Cyg Second-epoch detections are separated by 2.0" and 7.1 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 | 21:44:49.72 +36:56:53.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:49.72 +36:56:53.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:49.72 +36:56:53.9: 14.02 +/- 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
target,2461185.8473,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.39CV 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 25.3473 2461185.8473 11.37 21:21:04.51 +40:28:37.5
85.46787 -6.61929 galactic Cyg Second-epoch detections are separated by 1.7" and 6.5 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 1965608314355046656 | 21:21:00.98 +40:28:37.0 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:04.51 +40:28:37.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:04.51 +40:28:37.5: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 1965608314355046656,2461185.8473,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1965608314355046656 20260525.3473 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 25.3473 2461185.8473 11.28 22:01:57.33 +35:42:30.3
88.32351 -15.53152 galactic Peg Second-epoch detections are separated by 1.7" and 7.3 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 J330.4699+35.6919 | 22:01:54.97 +35:41:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:57.33 +35:42:30.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:57.33 +35:42:30.3: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 J330.4699+35.6919,2461185.8473,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J330.4699+35.6919 20260525.3473 11.28CV 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 25.3473 2461185.8473 11.35 22:00:15.47 +42:40:23.2
92.46937 -9.85068 galactic Lac Second-epoch detections are separated by 1.0" and 6.9 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 | 22:00:15.47 +42:40:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:15.47 +42:40:23.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:15.47 +42:40:23.2: 13.74 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461185.8473,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.41 22:24:43.50 +41:45:09.0
95.68886 -13.22930 galactic Lac Second-epoch detections are separated by 0.3" and 7.4 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 J336.1950+41.7590 | 22:24:43.50 +41:45:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:43.50 +41:45:09.0: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:43.50 +41:45:09.0: 14.01 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 J336.1950+41.7590,2461185.8473,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.1950+41.7590 20260525.3473 11.41CV 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 25.3473 2461185.8473 11.40 21:27:59.74 +37:32:17.8
84.33439 -9.64981 galactic Cyg Second-epoch detections are separated by 1.6" and 6.7 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 | 21:27:59.74 +37:32:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:59.74 +37:32:17.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:59.74 +37:32:17.8: 13.73 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461185.8473,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.57 21:12:46.98 +42:24:03.8
85.77528 -4.16526 galactic Cyg Second-epoch detections are separated by 1.5" and 6.8 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 J318.1903+42.4041 | 21:12:43.63 +42:24:23.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:46.98 +42:24:03.8: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:46.98 +42:24:03.8: 13.82 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 J318.1903+42.4041,2461185.8473,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.1903+42.4041 20260525.3473 11.57CV 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 25.3473 2461185.8473 11.36 21:14:14.01 +36:03:26.7
81.31237 -8.71104 galactic Cyg Second-epoch detections are separated by 1.7" and 6.9 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 | 21:14:14.01 +36:03:26.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:14.01 +36:03:26.7: 13.14 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:14.01 +36:03:26.7: 13.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.36 +/- 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,2461185.8473,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.36CV 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 25.3473 2461185.8473 11.46 21:17:06.42 +35:11:34.0
81.07888 -9.72860 galactic Cyg Second-epoch detections are separated by 1.5" and 7.1 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 J319.2861+35.2012 | 21:17:06.42 +35:11:34.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.673+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:06.42 +35:11:34.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:06.42 +35:11:34.0: 13.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 J319.2861+35.2012,2461185.8473,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.2861+35.2012 20260525.3473 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 25.3473 2461185.8473 11.27 22:26:17.45 +40:38:22.7
95.31887 -14.32295 galactic Lac Second-epoch detections are separated by 0.6" and 7.5 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 | 22:26:17.45 +40:38:22.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:17.45 +40:38:22.7: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:17.45 +40:38:22.7: 14.14 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461185.8473,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.54 21:42:23.05 +40:36:53.1
88.53116 -9.30240 galactic Cyg Second-epoch detections are separated by 1.3" and 7.0 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 J325.5857+40.6170 | 21:42:23.05 +40:36:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:23.05 +40:36:53.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:23.05 +40:36:53.1: 13.73 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J325.5857+40.6170,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.5857+40.6170 20260525.3473 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 25.3473 2461185.8473 11.34 22:05:53.83 +33:29:13.6
87.54981 -17.77710 galactic Peg Second-epoch detections are separated by 1.0" and 7.2 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 | 22:05:53.83 +33:29:13.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:53.83 +33:29:13.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:53.83 +33:29:13.6: 14.20 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.20 +/- 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,2461185.8473,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.52 22:02:27.71 +42:04:01.9
92.42048 -10.57906 galactic Lac Second-epoch detections are separated by 2.1" and 6.9 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 J330.6159+42.0668 | 22:02:27.71 +42:04:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:27.71 +42:04:01.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:27.71 +42:04:01.9: 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
ATO J330.6159+42.0668,2461185.8473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J330.6159+42.0668 20260525.3473 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 25.3473 2461185.8473 11.46 21:33:53.13 +33:18:17.1
82.19838 -13.52076 galactic Cyg Second-epoch detections are separated by 1.4" and 7.0 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 J323.4646+33.3036 | 21:33:51.31 +33:17:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:53.13 +33:18:17.1: 11.93 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:53.13 +33:18:17.1: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 J323.4646+33.3036,2461185.8473,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.4646+33.3036 20260525.3473 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 25.3473 2461185.8473 11.35 22:14:09.47 +38:28:27.7
92.06246 -14.79312 galactic Lac Second-epoch detections are separated by 1.3" and 7.5 pix
The object was found in VSX 4" Gaia DR3 1955341212206396160
Type: ROT
# Max. Min./Amp. JD0 Period
13.690 G 13.750 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:14:09.47 +38:28:27.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:14:09.47 +38:28:27.7: 13.83 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 1955341212206396160,2461185.8473,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1955341212206396160 20260525.3473 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 25.3473 2461185.8473 11.57 21:14:54.60 +34:58:50.3
80.60996 -9.54617 galactic Cyg Second-epoch detections are separated by 1.7" and 6.7 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 | 21:14:54.60 +34:58:50.3 (user input) | T | P | (position from user input) J-Ks=0.776+/-0.108 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:54.60 +34:58:50.3: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:54.60 +34:58:50.3: 13.67 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461185.8473,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.57CV 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 25.3473 2461185.8473 11.52 21:16:44.97 +34:40:58.5
80.65140 -10.02519 galactic Cyg Second-epoch detections are separated by 2.1" and 7.3 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 J319.1792+34.6852 | 21:16:41.99 +34:40:42.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:44.97 +34:40:58.5: 13.00 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:44.97 +34:40:58.5: 13.60 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 J319.1792+34.6852,2461185.8473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1792+34.6852 20260525.3473 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 25.3473 2461185.8473 11.41 21:12:59.88 +36:04:17.9
81.15097 -8.51848 galactic Cyg Second-epoch detections are separated by 2.8" and 6.7 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 1867715731811717760 | 21:12:57.67 +36:04:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:59.88 +36:04:17.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:59.88 +36:04:17.9: 13.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 1867715731811717760,2461185.8473,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1867715731811717760 20260525.3473 11.41CV 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 25.3473 2461185.8473 11.53 21:24:11.07 +37:39:45.7
83.88007 -9.02985 galactic Cyg Second-epoch detections are separated by 1.4" and 6.9 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 J321.0544+37.6627 | 21:24:11.07 +37:39:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.702+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:11.07 +37:39:45.7: 12.13 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:11.07 +37:39:45.7: 13.87 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 J321.0544+37.6627,2461185.8473,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.0544+37.6627 20260525.3473 11.53CV 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 25.3473 2461185.8473 11.51 22:17:45.88 +39:00:20.5
92.97364 -14.76564 galactic Lac Second-epoch detections are separated by 3.8" and 7.6 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 J334.4301+38.9974 | 22:17:45.88 +39:00:20.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.695+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:45.88 +39:00:20.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:45.88 +39:00:20.5: 14.36 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 J334.4301+38.9974,2461185.8473,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J334.4301+38.9974 20260525.3473 11.51CV 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 25.3473 2461185.8473 11.63 21:18:02.81 +41:31:39.7
85.82071 -5.47601 galactic Cyg Second-epoch detections are separated by 1.4" and 6.9 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 1968848605175366784 | 21:18:05.71 +41:31:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:02.81 +41:31:39.7: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:02.81 +41:31:39.7: 13.93 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 1968848605175366784,2461185.8473,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1968848605175366784 20260525.3473 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 25.3473 2461185.8473 11.65 21:39:02.90 +40:22:35.9
87.89151 -9.05715 galactic Cyg Second-epoch detections are separated by 1.7" and 6.7 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 | 21:39:02.90 +40:22:35.9 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:02.90 +40:22:35.9: 12.45 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:02.90 +40:22:35.9: 13.75 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461185.8473,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.50 22:05:01.96 +41:27:41.8
92.43541 -11.35127 galactic Lac Second-epoch detections are separated by 0.3" and 7.0 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 J331.2733+41.4646 | 22:05:01.96 +41:27:41.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.327+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:01.96 +41:27:41.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:01.96 +41:27:41.8: 14.04 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 J331.2733+41.4646,2461185.8473,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.2733+41.4646 20260525.3473 11.50CV 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 25.3473 2461185.8473 11.66 21:13:09.70 +38:07:24.2
82.68990 -7.14497 galactic Cyg Second-epoch detections are separated by 1.4" and 7.0 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 J318.2909+38.1159 | 21:13:09.70 +38:07:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.447+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:09.70 +38:07:24.2: 12.86 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:09.70 +38:07:24.2: 13.95 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J318.2909+38.1159,2461185.8473,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.2909+38.1159 20260525.3473 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 25.3473 2461185.8473 11.63 21:28:41.55 +42:35:38.9
87.98473 -6.11294 galactic Cyg Second-epoch detections are separated by 1.8" and 6.9 pix
The object was found in VSX 5" ASASSN-V J212841.45+423543.6
Type: SR
# Max. Min./Amp. JD0 Period
15.370 g Y 0.290 g 2458319.89600 581.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:41.55 +42:35:38.9: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:41.55 +42:35:38.9: 14.00 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 J212841.45+423543.6,2461185.8473,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212841.45+423543.6 20260525.3473 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 25.3473 2461185.8473 11.63 21:26:50.82 +42:27:02.6
87.63858 -5.97987 galactic Cyg Second-epoch detections are separated by 1.4" and 6.5 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 1967445903224193920 | 21:26:46.91 +42:27:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:50.82 +42:27:02.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:50.82 +42:27:02.6: 13.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 1967445903224193920,2461185.8473,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1967445903224193920 20260525.3473 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 25.3473 2461185.8473 11.52 21:16:35.26 +37:06:18.1
82.41124 -8.33707 galactic Cyg Second-epoch detections are separated by 1.7" and 7.0 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 1868617851048487424 | 21:16:32.71 +37:06:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:35.26 +37:06:18.1: 12.04 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:35.26 +37:06:18.1: 13.61 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 1868617851048487424,2461185.8473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868617851048487424 20260525.3473 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 25.3473 2461185.8473 11.55 21:58:13.38 +38:26:14.2
89.48126 -12.93506 galactic Lac Second-epoch detections are separated by 2.3" and 7.5 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 J329.5588+38.4358 | 21:58:13.38 +38:26:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:13.38 +38:26:14.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:13.38 +38:26:14.2: 14.06 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 J329.5588+38.4358,2461185.8473,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.5588+38.4358 20260525.3473 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 25.3473 2461185.8473 11.54 22:15:17.49 +39:47:51.6
93.03975 -13.84295 galactic Lac Second-epoch detections are separated by 1.7" and 7.5 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 | 22:15:17.49 +39:47:51.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:15:17.49 +39:47:51.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:15:17.49 +39:47:51.6: 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
target,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.56 21:15:47.41 +37:50:42.3
82.84340 -7.71290 galactic Cyg Second-epoch detections are separated by 1.6" and 7.1 pix
The object was found in VSX 3" ASASSN-V J211547.60+375039.7
Type: EA
# Max. Min./Amp. JD0 Period
14.230 V 14.380 V 2457586.90800 2.353500000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:47.41 +37:50:42.3: 12.37 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:47.41 +37:50:42.3: 14.05 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 J211547.60+375039.7,2461185.8473,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J211547.60+375039.7 20260525.3473 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 25.3473 2461185.8473 11.54 21:12:44.35 +36:07:58.7
81.16057 -8.43845 galactic Cyg Second-epoch detections are separated by 2.6" and 6.6 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 J318.1899+36.1280 | 21:12:44.35 +36:07:58.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.203+/-0.063 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:44.35 +36:07:58.7: 12.87 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:44.35 +36:07:58.7: 14.06 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 J318.1899+36.1280,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.1899+36.1280 20260525.3473 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 25.3473 2461185.8473 11.62 21:18:43.48 +37:57:52.4
83.33448 -8.04863 galactic Cyg Second-epoch detections are separated by 2.1" and 7.2 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 1964745541325117184 | 21:18:46.39 +37:57:56.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.345+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:43.48 +37:57:52.4: 12.92 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:43.48 +37:57:52.4: 13.99 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 1964745541325117184,2461185.8473,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1964745541325117184 20260525.3473 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 25.3473 2461185.8473 11.68 21:13:16.20 +41:07:40.5
84.90803 -5.10437 galactic Cyg Second-epoch detections are separated by 4.2" and 6.4 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 J318.3318+41.1436 | 21:13:19.29 +41:08:10.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.596+/-0.050 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:16.20 +41:07:40.5: 12.92 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:16.20 +41:07:40.5: 13.81 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J318.3318+41.1436,2461185.8473,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.3318+41.1436 20260525.3473 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 25.3473 2461185.8473 11.60 22:02:04.51 +37:45:26.1
89.65655 -13.93892 galactic Lac Second-epoch detections are separated by 0.4" and 7.1 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 | 22:02:04.51 +37:45:26.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:04.51 +37:45:26.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:04.51 +37:45:26.1: 14.34 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461185.8473,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.69 22:05:11.22 +41:31:52.7
92.50176 -11.31305 galactic Lac Second-epoch detections are separated by 1.4" and 6.9 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 J331.2992+41.5224 | 22:05:09.23 +41:31:24.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:11.22 +41:31:52.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:11.22 +41:31:52.7: 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
ATO J331.2992+41.5224,2461185.8473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.2992+41.5224 20260525.3473 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 25.3473 2461185.8473 11.58 22:07:43.26 +37:37:03.4
90.48187 -14.73120 galactic Lac Second-epoch detections are separated by 2.2" and 7.4 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 | 22:07:43.26 +37:37:03.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:43.26 +37:37:03.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:43.26 +37:37:03.4: 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 J331.9384+37.6117,2461185.8473,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 11.58CV 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 25.3473 2461185.8473 11.54 21:50:11.43 +35:33:08.1
86.31555 -14.12741 galactic Peg Second-epoch detections are separated by 2.3" and 7.1 pix
The object was found in VSX 2" Gaia DR3 1949071109713094272
Type: ROT
# Max. Min./Amp. JD0 Period
13.850 G 13.890 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:11.43 +35:33:08.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:11.43 +35:33:08.1: 14.22 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.22 +/- 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
Gaia DR3 1949071109713094272,2461185.8473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1949071109713094272 20260525.3473 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 25.3473 2461185.8473 11.71 21:21:06.53 +36:01:47.5
82.26304 -9.73657 galactic Cyg Second-epoch detections are separated by 0.9" and 7.1 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 J320.2783+36.0305 | 21:21:06.53 +36:01:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:06.53 +36:01:47.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:06.53 +36:01:47.5: 14.07 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 J320.2783+36.0305,2461185.8473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.2783+36.0305 20260525.3473 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 25.3473 2461185.8473 11.73 21:24:57.22 +42:40:16.6
87.54292 -5.57846 galactic Cyg Second-epoch detections are separated by 4.9" and 7.4 pix
The object was found in VSX 4" ASASSN-V J212457.56+424016.6
Type: SR
# Max. Min./Amp. JD0 Period
14.920 V 15.260 V 2457927.06000 62.460000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:57.22 +42:40:16.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:57.22 +42:40:16.6: 14.42 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.42 +/- 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
ASASSN-V J212457.56+424016.6,2461185.8473,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212457.56+424016.6 20260525.3473 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 25.3473 2461185.8473 11.74 21:11:38.29 +37:30:37.3
82.03070 -7.34168 galactic Cyg Second-epoch detections are separated by 1.9" and 7.0 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 J317.9122+37.5128 | 21:11:38.29 +37:30:37.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.358+/-0.066 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:38.29 +37:30:37.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:38.29 +37:30:37.3: 14.11 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 J317.9122+37.5128,2461185.8473,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.9122+37.5128 20260525.3473 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 25.3473 2461185.8473 11.59 22:12:04.42 +37:38:52.8
91.21635 -15.22122 galactic Lac Second-epoch detections are separated by 6.7" and 7.6 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 | 22:12:04.42 +37:38:52.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:04.42 +37:38:52.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:04.42 +37:38:52.8: 14.50 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.50 +/- 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,2461185.8473,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.59CV 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 25.3473 2461185.8473 11.81 21:39:47.29 +42:43:07.2
89.57721 -7.40757 galactic Cyg Second-epoch detections are separated by 3.7" and 6.2 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 1966913400297365632 | 21:39:45.67 +42:42:28.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:47.29 +42:43:07.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:47.29 +42:43:07.2: 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 1966913400297365632,2461185.8473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1966913400297365632 20260525.3473 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 25.3473 2461185.8473 11.62 21:29:32.10 +33:48:17.3
81.89196 -12.52958 galactic Cyg Second-epoch detections are separated by 2.2" and 6.9 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 | 21:29:32.10 +33:48:17.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:32.10 +33:48:17.3: 11.79 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:32.10 +33:48:17.3: 14.08 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.65 +/- 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,2461185.8473,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.69 22:21:24.16 +41:17:43.9
94.89705 -13.26759 galactic Lac Second-epoch detections are separated by 3.4" and 7.6 pix
The object was found in VSX 4" Gaia DR3 1957666266982423552
Type: VAR
# Max. Min./Amp. JD0 Period
14.670 G 14.730 G 0.521140000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:24.16 +41:17:43.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:24.16 +41:17:43.9: 14.66 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.66 +/- 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 1957666266982423552,2461185.8473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957666266982423552 20260525.3473 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 25.3473 2461185.8473 11.70 22:13:03.48 +38:28:18.8
91.88042 -14.66923 galactic Lac Second-epoch detections are separated by 3.1" and 6.8 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 | 22:13:03.48 +38:28:18.8 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:13:03.48 +38:28:18.8: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:13:03.48 +38:28:18.8: 14.01 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461185.8473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.59 22:09:23.69 +40:29:36.8
92.51892 -12.61945 galactic Lac Second-epoch detections are separated by 0.5" and 7.1 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 1956516074742793344 | 22:09:25.55 +40:29:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:23.69 +40:29:36.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:23.69 +40:29:36.8: 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 1956516074742793344,2461185.8473,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1956516074742793344 20260525.3473 11.59CV 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 25.3473 2461185.8473 11.61 22:17:25.04 +42:04:44.7
94.71734 -12.20138 galactic Lac Second-epoch detections are separated by 4.7" and 6.5 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 1958148780790359552 | 22:17:21.78 +42:04:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:25.04 +42:04:44.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:25.04 +42:04:44.7: 13.97 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 1958148780790359552,2461185.8473,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1958148780790359552 20260525.3473 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 25.3473 2461185.8473 11.69 21:13:58.07 +36:59:38.7
81.96749 -8.03272 galactic Cyg Second-epoch detections are separated by 2.3" and 6.9 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 J318.4959+36.9962 | 21:13:58.07 +36:59:38.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:58.07 +36:59:38.7: 12.12 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:58.07 +36:59:38.7: 14.12 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.02 +/- 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
ATO J318.4959+36.9962,2461185.8473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.4959+36.9962 20260525.3473 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 25.3473 2461185.8473 11.85 21:17:44.76 +38:40:34.1
83.71721 -7.41668 galactic Cyg Second-epoch detections are separated by 1.2" and 6.9 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 J319.4539+38.6736 | 21:17:47.23 +38:40:36.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:44.76 +38:40:34.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:44.76 +38:40:34.1: 13.80 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 J319.4539+38.6736,2461185.8473,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.4539+38.6736 20260525.3473 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 25.3473 2461185.8473 11.71 21:17:03.32 +37:35:40.5
82.83421 -8.06682 galactic Cyg Second-epoch detections are separated by 1.1" and 6.9 pix
The object was found in VSX25" Gaia DR3 1964722279780956800
Type: E
# Max. Min./Amp. JD0 Period
17.040 G 17.380 G 2.450630000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:03.32 +37:35:40.5: 12.94 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:03.32 +37:35:40.5: 14.02 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 1964722279780956800,2461185.8473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1964722279780956800 20260525.3473 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 25.3473 2461185.8473 11.80 21:14:34.90 +37:36:52.5
82.50874 -7.69737 galactic Cyg Second-epoch detections are separated by 3.8" and 7.1 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 J318.6352+37.6074 | 21:14:34.90 +37:36:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.712+/-0.311 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:34.90 +37:36:52.5: 12.80 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:34.90 +37:36:52.5: 14.01 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 J318.6352+37.6074,2461185.8473,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.6352+37.6074 20260525.3473 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 25.3473 2461185.8473 11.93 21:18:25.07 +38:04:45.1
83.37544 -7.92556 galactic Cyg Second-epoch detections are separated by 0.4" and 6.8 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 J319.6016+38.0792 | 21:18:25.07 +38:04:45.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:25.07 +38:04:45.1: 12.92 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:25.07 +38:04:45.1: 14.66 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 J319.6016+38.0792,2461185.8473,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.6016+38.0792 20260525.3473 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 25.3473 2461185.8473 11.75 21:34:59.13 +39:59:54.0
87.05378 -8.81157 galactic Cyg Second-epoch detections are separated by 2.5" and 6.4 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 1966034375107416320 | 21:35:01.94 +39:59:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.951+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:59.13 +39:59:54.0: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:59.13 +39:59:54.0: 14.47 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.47 +/- 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
Gaia DR3 1966034375107416320,2461185.8473,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1966034375107416320 20260525.3473 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 25.3473 2461185.8473 11.87 21:09:58.24 +38:52:34.6
82.81896 -6.17535 galactic Cyg Second-epoch detections are separated by 2.0" and 6.9 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 | 21:09:58.24 +38:52:34.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:58.24 +38:52:34.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:58.24 +38:52:34.6: 14.16 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.16 +/- 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,2461185.8473,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.65 21:37:54.69 +33:00:12.4
82.61166 -14.32071 galactic Cyg Second-epoch detections are separated by 1.7" and 7.4 pix
The object was found in VSX 4" Gaia DR3 1947030656652560768
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.060 G 14.110 G 0.184640200000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:54.69 +33:00:12.4: 12.74 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:54.69 +33:00:12.4: 14.20 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 1947030656652560768,2461185.8473,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1947030656652560768 20260525.3473 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 25.3473 2461185.8473 11.64 21:59:59.93 +38:42:23.1
89.93187 -12.94119 galactic Lac Second-epoch detections are separated by 1.2" and 7.1 pix
The object was found in VSX20" Gaia DR3 1956026134933788544
Type: ROT
# Max. Min./Amp. JD0 Period
18.080 G 18.230 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:59.93 +38:42:23.1: 13.34 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:59.93 +38:42:23.1: 14.21 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.08 +/- 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 1956026134933788544,2461185.8473,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1956026134933788544 20260525.3473 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3473 2461185.8473 11.75 21:17:15.71 +34:09:14.6
80.33374 -10.46467 galactic Cyg Second-epoch detections are separated by 0.5" and 7.0 pix
The object was found in VSX 6" Gaia DR3 1855293969141296000
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.440 G 14.480 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:15.71 +34:09:14.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:15.71 +34:09:14.6: 14.26 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.26 +/- 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 1855293969141296000,2461185.8473,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1855293969141296000 20260525.3473 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 25.3473 2461185.8473 11.78 22:21:51.89 +38:05:41.0
93.12271 -15.97055 galactic Lac Second-epoch detections are separated by 8.5" and 6.2 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 J335.4606+38.0846 | 22:21:51.89 +38:05:41.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:51.89 +38:05:41.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:51.89 +38:05:41.0: 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
ATO J335.4606+38.0846,2461185.8473,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.4606+38.0846 20260525.3473 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 25.3473 2461185.8473 11.76 21:56:32.95 +38:17:22.8
89.12430 -12.84361 galactic Cyg Second-epoch detections are separated by 1.4" and 7.0 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 | 21:56:32.95 +38:17:22.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:32.95 +38:17:22.8: 12.85 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:32.95 +38:17:22.8: 14.20 +/- 0.10 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,2461185.8473,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.99 21:21:53.02 +41:39:20.3
86.41784 -5.89784 galactic Cyg Second-epoch detections are separated by 0.9" and 6.7 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 J320.4698+41.6545 | 21:21:53.02 +41:39:20.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:53.02 +41:39:20.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:53.02 +41:39:20.3: 14.16 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J320.4698+41.6545,2461185.8473,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.4698+41.6545 20260525.3473 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 25.3473 2461185.8473 11.78 22:05:11.01 +42:22:39.9
93.01982 -10.63644 galactic Lac Second-epoch detections are separated by 1.5" and 7.2 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 J331.2712+42.3814 | 22:05:07.54 +42:22:18.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:11.01 +42:22:39.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:11.01 +42:22:39.9: 14.48 +/- 0.17 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
ATO J331.2712+42.3814,2461185.8473,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J331.2712+42.3814 20260525.3473 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 25.3473 2461185.8473 11.83 21:42:23.52 +41:49:36.8
89.34384 -8.39440 galactic Cyg Second-epoch detections are separated by 0.7" and 6.8 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 | 21:42:23.52 +41:49:36.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:23.52 +41:49:36.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:23.52 +41:49:36.8: 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
target,2461185.8473,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.67 22:19:20.15 +40:03:19.4
93.84720 -14.07438 galactic Lac Second-epoch detections are separated by 0.7" and 7.4 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 | 22:19:20.15 +40:03:19.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:20.15 +40:03:19.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:20.15 +40:03:19.4: 14.08 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461185.8473,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.70 21:57:59.24 +41:37:13.3
91.47272 -10.41886 galactic Lac Second-epoch detections are separated by 1.1" and 7.1 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 1959984174936797696 | 21:57:55.98 +41:36:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:59.24 +41:37:13.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:59.24 +41:37:13.3: 14.07 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 1959984174936797696,2461185.8473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1959984174936797696 20260525.3473 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 25.3473 2461185.8473 11.83 21:19:28.79 +39:57:40.4
84.88240 -6.76330 galactic Cyg Second-epoch detections are separated by 2.2" and 6.8 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 J319.8668+39.9566 | 21:19:28.79 +39:57:40.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.748+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:28.79 +39:57:40.4: 13.29 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:28.79 +39:57:40.4: 14.36 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 J319.8668+39.9566,2461185.8473,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.8668+39.9566 20260525.3473 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 25.3473 2461185.8473 11.79 21:14:51.36 +38:32:19.8
83.22432 -7.10274 galactic Cyg Second-epoch detections are separated by 1.3" and 6.5 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 J318.7293+38.5358 | 21:14:51.36 +38:32:19.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.766+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:51.36 +38:32:19.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:51.36 +38:32:19.8: 14.18 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 J318.7293+38.5358,2461185.8473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.7293+38.5358 20260525.3473 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 25.3473 2461185.8473 11.99 21:09:53.82 +42:17:25.4
85.32943 -3.85094 galactic Cyg Second-epoch detections are separated by 2.3" and 6.3 pix
The object was found in VSX18" Gaia DR3 1969832775471453056
Type: S
# Max. Min./Amp. JD0 Period
18.560 G 19.510 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:53.82 +42:17:25.4: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:53.82 +42:17:25.4: 14.45 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 1969832775471453056,2461185.8473,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1969832775471453056 20260525.3473 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 25.3473 2461185.8473 11.85 21:11:50.84 +40:34:54.6
84.32325 -5.28161 galactic Cyg Second-epoch detections are separated by 1.9" and 6.4 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 | 21:11:50.84 +40:34:54.6 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:50.84 +40:34:54.6: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:50.84 +40:34:54.6: 14.27 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461185.8473,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.82 21:27:09.80 +36:53:13.9
83.75095 -9.99750 galactic Cyg Second-epoch detections are separated by 3.7" and 6.3 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 1951737902147573376 | 21:27:12.98 +36:53:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:09.80 +36:53:13.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:09.80 +36:53:13.9: 13.94 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 1951737902147573376,2461185.8473,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1951737902147573376 20260525.3473 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 25.3473 2461185.8473 11.76 22:12:26.42 +40:34:53.0
93.05169 -12.88872 galactic Lac Second-epoch detections are separated by 4.2" and 7.8 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 | 22:12:26.42 +40:34:53.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:26.42 +40:34:53.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:26.42 +40:34:53.0: 15.13 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.13 +/- 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,2461185.8473,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.83 21:14:03.36 +34:52:46.8
80.41412 -9.48676 galactic Cyg Second-epoch detections are separated by 2.0" and 7.2 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 J318.5050+34.8760 | 21:14:03.36 +34:52:46.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:03.36 +34:52:46.8: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:03.36 +34:52:46.8: 13.91 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 J318.5050+34.8760,2461185.8473,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.5050+34.8760 20260525.3473 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 25.3473 2461185.8473 11.64 22:09:11.24 +36:46:05.1
90.19377 -15.58539 galactic Lac Second-epoch detections are separated by 2.7" and 7.6 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 J332.2936+36.7689 | 22:09:11.24 +36:46:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:11.24 +36:46:05.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:11.24 +36:46:05.1: 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
ATO J332.2936+36.7689,2461185.8473,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3473 2461185.8473 11.83 21:14:10.55 +37:06:09.0
82.07607 -7.98896 galactic Cyg Second-epoch detections are separated by 2.4" and 6.9 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 J318.5475+37.1028 | 21:14:10.55 +37:06:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.277+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:10.55 +37:06:09.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:10.55 +37:06:09.0: 14.18 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 J318.5475+37.1028,2461185.8473,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.5475+37.1028 20260525.3473 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 25.3473 2461185.8473 11.72 21:36:48.43 +38:51:41.5
86.53241 -9.88460 galactic Cyg Second-epoch detections are separated by 1.9" and 6.6 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 J324.1997+38.8630 | 21:36:48.43 +38:51:41.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:48.43 +38:51:41.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:48.43 +38:51:41.5: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 J324.1997+38.8630,2461185.8473,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.1997+38.8630 20260525.3473 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 25.3473 2461185.8473 11.68 21:10:24.23 +38:26:35.0
82.55556 -6.53074 galactic Cyg Second-epoch detections are separated by 1.1" and 6.8 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 | 21:10:24.23 +38:26:35.0 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:24.23 +38:26:35.0: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:24.23 +38:26:35.0: 13.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461185.8473,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.72 22:04:36.81 +38:54:14.7
90.78473 -13.33810 galactic Lac Second-epoch detections are separated by 2.1" and 7.3 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 1955939827569816448 | 22:04:34.49 +38:53:59.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:36.81 +38:54:14.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:36.81 +38:54:14.7: 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
Gaia DR3 1955939827569816448,2461185.8473,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1955939827569816448 20260525.3473 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 25.3473 2461185.8473 11.83 21:37:35.64 +40:12:05.7
87.56449 -9.00015 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 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 1966017367036446848 | 21:37:38.47 +40:11:37.7 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:35.64 +40:12:05.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:35.64 +40:12:05.7: 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
Gaia DR3 1966017367036446848,2461185.8473,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1966017367036446848 20260525.3473 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 25.3473 2461185.8473 11.81 21:11:38.47 +38:20:47.4
82.64965 -6.77439 galactic Cyg Second-epoch detections are separated by 1.2" and 6.5 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 J317.9161+38.3399 | 21:11:38.47 +38:20:47.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:38.47 +38:20:47.4: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:38.47 +38:20:47.4: 14.24 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 J317.9161+38.3399,2461185.8473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.9161+38.3399 20260525.3473 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 25.3473 2461185.8473 11.78 21:27:12.32 +39:44:01.5
85.77699 -7.97297 galactic Cyg Second-epoch detections are separated by 1.6" and 6.9 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 | 21:27:12.32 +39:44:01.5 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:12.32 +39:44:01.5: 12.70 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:12.32 +39:44:01.5: 14.35 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461185.8473,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.90 21:12:24.20 +40:10:31.1
84.09741 -5.63648 galactic Cyg Second-epoch detections are separated by 3.3" and 6.2 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 | 21:12:24.20 +40:10:31.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:24.20 +40:10:31.1: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:24.20 +40:10:31.1: 13.75 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461185.8473,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.87 21:14:41.33 +34:18:39.8
80.08115 -9.96902 galactic Cyg Second-epoch detections are separated by 2.4" and 6.6 pix
The object was found in VSX 1" ASASSN-V J211441.29+341839.5
Type: VAR
# Max. Min./Amp. JD0 Period
15.100 V 15.900 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:41.33 +34:18:39.8: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:41.33 +34:18:39.8: 14.63 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.63 +/- 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
ASASSN-V J211441.29+341839.5,2461185.8473,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J211441.29+341839.5 20260525.3473 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 25.3473 2461185.8473 11.74 21:14:48.66 +37:08:03.6
82.18700 -8.05952 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 | 21:14:48.66 +37:08:03.6 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:48.66 +37:08:03.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:48.66 +37:08:03.6: 13.90 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.90 +/- 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,2461185.8473,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.94 21:20:06.58 +39:26:52.7
84.59785 -7.20864 galactic Cyg Second-epoch detections are separated by 4.4" and 6.0 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 | 21:20:06.58 +39:26:52.7 (user input) | T | P | (position from user input) J-Ks=0.974+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:06.58 +39:26:52.7: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:06.58 +39:26:52.7: 13.99 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461185.8473,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.73 21:36:15.14 +40:02:53.3
87.26815 -8.93978 galactic Cyg Second-epoch detections are separated by 1.6" and 6.8 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 J324.0798+40.0481 | 21:36:17.72 +40:02:25.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:15.14 +40:02:53.3: 12.93 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:15.14 +40:02:53.3: 14.04 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 J324.0798+40.0481,2461185.8473,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.0798+40.0481 20260525.3473 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 25.3473 2461185.8473 11.91 21:11:51.11 +35:37:58.7
80.66562 -8.64518 galactic Cyg Second-epoch detections are separated by 3.3" and 7.1 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 | 21:11:51.11 +35:37:58.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:51.11 +35:37:58.7: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:51.11 +35:37:58.7: 14.47 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.47 +/- 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,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.86 21:18:55.54 +41:30:47.1
85.92551 -5.60405 galactic Cyg Second-epoch detections are separated by 4.0" and 6.6 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 J319.7251+41.5048 | 21:18:55.54 +41:30:47.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.793+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:55.54 +41:30:47.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:55.54 +41:30:47.1: 14.35 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.35 +/- 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 J319.7251+41.5048,2461185.8473,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.7251+41.5048 20260525.3473 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 25.3473 2461185.8473 12.03 21:14:40.80 +39:49:56.5
84.14675 -6.18900 galactic Cyg Second-epoch detections are separated by 1.4" and 6.4 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 | 21:14:40.80 +39:49:56.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:40.80 +39:49:56.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:40.80 +39:49:56.5: 14.35 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.35 +/- 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,2461185.8473,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.93 21:11:58.18 +34:50:23.8
80.09054 -9.19900 galactic Cyg Second-epoch detections are separated by 5.4" and 7.9 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 | 21:11:58.18 +34:50:23.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:58.18 +34:50:23.8: 12.69 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:58.18 +34:50:23.8: 14.23 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461185.8473,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.71 21:34:11.25 +40:41:03.1
87.41375 -8.20594 galactic Cyg Second-epoch detections are separated by 5.4" and 7.1 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 1966258469323454976 | 21:34:14.26 +40:40:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.158+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:11.25 +40:41:03.1: 11.98 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:11.25 +40:41:03.1: 14.07 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 1966258469323454976,2461185.8473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1966258469323454976 20260525.3473 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 25.3473 2461185.8473 11.79 21:14:07.41 +39:48:24.2
84.05417 -6.12898 galactic Cyg Second-epoch detections are separated by 2.3" and 6.3 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 J318.5283+39.8132 | 21:14:07.41 +39:48:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:07.41 +39:48:24.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:07.41 +39:48:24.2: 14.20 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.20 +/- 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 J318.5283+39.8132,2461185.8473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.5283+39.8132 20260525.3473 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 25.3473 2461185.8473 11.95 21:17:15.26 +35:51:06.5
81.58491 -9.29716 galactic Cyg Second-epoch detections are separated by 2.8" and 6.6 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 J319.3154+35.8532 | 21:17:15.26 +35:51:06.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.416+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:15.26 +35:51:06.5: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:15.26 +35:51:06.5: 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
ATO J319.3154+35.8532,2461185.8473,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3154+35.8532 20260525.3473 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 25.3473 2461185.8473 11.90 21:29:00.59 +35:14:11.5
82.84140 -11.43461 galactic Cyg Second-epoch detections are separated by 6.9" and 7.5 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 | 21:29:00.59 +35:14:11.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:00.59 +35:14:11.5: 12.96 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:00.59 +35:14:11.5: 14.31 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461185.8473,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.86 21:15:07.43 +38:34:26.4
83.28633 -7.11663 galactic Cyg Second-epoch detections are separated by 0.7" and 6.7 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 | 21:15:07.43 +38:34:26.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:07.43 +38:34:26.4: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:07.43 +38:34:26.4: 14.03 +/- 0.13 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,2461185.8473,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.13 21:19:18.15 +42:26:13.0
86.63775 -5.00782 galactic Cyg Second-epoch detections are separated by 1.5" and 6.4 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 | 21:19:18.15 +42:26:13.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:18.15 +42:26:13.0: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:18.15 +42:26:13.0: 14.35 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.35 +/- 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,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.77 22:01:03.93 +41:04:56.1
91.59684 -11.19885 galactic Lac Second-epoch detections are separated by 2.5" and 6.7 pix
The object was found in VSX 3" 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:03.93 +41:04:56.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:03.93 +41:04:56.1: 13.93 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 1959714932024123904,2461185.8473,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 11.96 21:22:28.29 +40:43:48.8
85.83670 -6.62922 galactic Cyg Second-epoch detections are separated by 1.3" and 6.8 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 J320.6273+40.7307 | 21:22:28.29 +40:43:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:28.29 +40:43:48.8: 13.20 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:28.29 +40:43:48.8: 14.19 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 J320.6273+40.7307,2461185.8473,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.6273+40.7307 20260525.3473 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 25.3473 2461185.8473 12.06 21:19:19.25 +39:41:30.2
84.66660 -6.92959 galactic Cyg Second-epoch detections are separated by 4.4" and 6.0 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 | 21:19:19.25 +39:41:30.2 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:19.25 +39:41:30.2: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:19.25 +39:41:30.2: 14.36 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461185.8473,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.86 21:56:00.37 +37:10:55.8
88.31903 -13.63332 galactic Cyg Second-epoch detections are separated by 2.9" and 6.7 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 | 21:56:00.37 +37:10:55.8 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:00.37 +37:10:55.8: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:00.37 +37:10:55.8: 14.44 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.44 +/- 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,2461185.8473,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.92 21:12:39.54 +38:09:44.1
82.65061 -7.04619 galactic Cyg Second-epoch detections are separated by 1.9" and 6.5 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 J318.1558+38.1707 | 21:12:39.54 +38:09:44.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.329+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:39.54 +38:09:44.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:39.54 +38:09:44.1: 14.23 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.23 +/- 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 J318.1558+38.1707,2461185.8473,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.1558+38.1707 20260525.3473 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3473 2461185.8473 11.79 21:43:36.58 +42:31:44.2
89.98261 -8.01484 galactic Cyg Second-epoch detections are separated by 1.3" and 7.0 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 J325.9048+42.5318 | 21:43:36.58 +42:31:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:36.58 +42:31:44.2: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:36.58 +42:31:44.2: 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
ATO J325.9048+42.5318,2461185.8473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.9048+42.5318 20260525.3473 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 25.3473 2461185.8473 11.91 21:11:33.88 +36:22:57.6
81.18383 -8.09512 galactic Cyg Second-epoch detections are separated by 2.5" and 6.5 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 J317.8793+36.3802 | 21:11:33.88 +36:22:57.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:33.88 +36:22:57.6: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:33.88 +36:22:57.6: 15.01 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.01 +/- 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
ATO J317.8793+36.3802,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.8793+36.3802 20260525.3473 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 25.3473 2461185.8473 11.88 21:12:04.94 +42:34:05.0
85.80857 -3.95676 galactic Cyg Second-epoch detections are separated by 0.9" and 6.5 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 J318.0205+42.5689 | 21:12:04.94 +42:34:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:04.94 +42:34:05.0: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:04.94 +42:34:05.0: 14.23 +/- 0.17 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
ATO J318.0205+42.5689,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.0205+42.5689 20260525.3473 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 25.3473 2461185.8473 12.09 21:17:15.27 +41:40:01.8
85.81775 -5.27258 galactic Cyg Second-epoch detections are separated by 1.5" and 6.4 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 J319.3098+41.6676 | 21:17:15.27 +41:40:01.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.441+/-0.051 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:15.27 +41:40:01.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:15.27 +41:40:01.8: 14.09 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 J319.3098+41.6676,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3098+41.6676 20260525.3473 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 25.3473 2461185.8473 12.05 21:26:38.61 +39:47:22.1
85.73845 -7.85762 galactic Cyg Second-epoch detections are separated by 2.4" and 7.1 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 | 21:26:38.61 +39:47:22.1 (user input) | T | P | (position from user input) J-Ks=0.915+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:38.61 +39:47:22.1: 13.26 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:38.61 +39:47:22.1: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.29 +/- 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,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.02 21:24:42.39 +38:26:36.8
84.51238 -8.55046 galactic Cyg Second-epoch detections are separated by 3.6" and 7.3 pix
The object was found in VSX 4" ASASSN-V J212442.51+382640.2
Type: M
# Max. Min./Amp. JD0 Period
20.450 g Y 4.379 g 2458324.51660 375.299483000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:42.39 +38:26:36.8: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:42.39 +38:26:36.8: 15.24 +/- 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
ASASSN-V J212442.51+382640.2,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212442.51+382640.2 20260525.3473 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 25.3473 2461185.8473 12.09 21:16:06.05 +38:52:02.3
83.63288 -7.05285 galactic Cyg Second-epoch detections are separated by 1.3" and 7.0 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 J319.0252+38.8786 | 21:16:06.05 +38:52:02.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.761+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:06.05 +38:52:02.3: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:06.05 +38:52:02.3: 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
ATO J319.0252+38.8786,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.0252+38.8786 20260525.3473 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 25.3473 2461185.8473 11.88 21:16:22.33 +37:47:56.0
82.88946 -7.82805 galactic Cyg Second-epoch detections are separated by 2.0" and 6.5 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 J319.0855+37.8028 | 21:16:22.33 +37:47:56.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.633+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:22.33 +37:47:56.0: 13.16 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:22.33 +37:47:56.0: 14.43 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J319.0855+37.8028,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.0855+37.8028 20260525.3473 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 25.3473 2461185.8473 12.04 21:09:04.49 +40:48:05.6
84.12686 -4.74663 galactic Cyg Second-epoch detections are separated by 1.8" and 6.6 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 | 21:09:04.49 +40:48:05.6 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:04.49 +40:48:05.6: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:04.49 +40:48:05.6: 14.28 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461185.8473,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.79 21:41:50.86 +35:55:28.9
85.26468 -12.72743 galactic Cyg Second-epoch detections are separated by 3.7" and 7.1 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 J325.4608+35.9170 | 21:41:50.86 +35:55:28.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:50.86 +35:55:28.9: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:50.86 +35:55:28.9: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 J325.4608+35.9170,2461185.8473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.4608+35.9170 20260525.3473 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 25.3473 2461185.8473 11.91 21:46:53.87 +39:15:18.7
88.28450 -10.89550 galactic Cyg Second-epoch detections are separated by 2.0" and 6.8 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 | 21:46:53.87 +39:15:18.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:53.87 +39:15:18.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:53.87 +39:15:18.7: 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,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.98 21:15:45.32 +36:35:09.8
81.91447 -8.57291 galactic Cyg Second-epoch detections are separated by 2.8" and 6.5 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 J318.9377+36.5866 | 21:15:45.32 +36:35:09.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:45.32 +36:35:09.8: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:45.32 +36:35:09.8: 14.17 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.17 +/- 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 J318.9377+36.5866,2461185.8473,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.9377+36.5866 20260525.3473 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 25.3473 2461185.8473 12.02 21:11:20.88 +39:12:54.3
83.25181 -6.14218 galactic Cyg Second-epoch detections are separated by 2.2" and 6.6 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 | 21:11:20.88 +39:12:54.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:20.88 +39:12:54.3: 12.69 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:20.88 +39:12:54.3: 14.24 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:12:38.13 +39:31:59.6
83.65651 -6.10755 galactic Cyg Second-epoch detections are separated by 3.0" and 7.2 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 | 21:12:38.13 +39:31:59.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:38.13 +39:31:59.6: 12.75 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:38.13 +39:31:59.6: 14.59 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.87 21:56:34.36 +37:00:25.9
88.29476 -13.84025 galactic Cyg Second-epoch detections are separated by 1.3" and 7.3 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 1949631375305780480 | 21:56:30.58 +37:00:26.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:34.36 +37:00:25.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:34.36 +37:00:25.9: 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
Gaia DR3 1949631375305780480,2461185.8473,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1949631375305780480 20260525.3473 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 25.3473 2461185.8473 12.03 21:15:01.14 +37:38:00.8
82.58258 -7.74742 galactic Cyg Second-epoch detections are separated by 3.5" and 6.4 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 | 21:15:01.14 +37:38:00.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:01.14 +37:38:00.8: 12.73 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:01.14 +37:38:00.8: 14.22 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461185.8473,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.02 21:19:04.73 +38:33:58.2
83.81981 -7.68035 galactic Cyg Second-epoch detections are separated by 2.6" and 6.4 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 J319.7665+38.5707 | 21:19:04.73 +38:33:58.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:04.73 +38:33:58.2: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:04.73 +38:33:58.2: 14.28 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 J319.7665+38.5707,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.7665+38.5707 20260525.3473 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 25.3473 2461185.8473 11.90 21:59:30.86 +42:08:23.4
92.02640 -10.18674 galactic Lac Second-epoch detections are separated by 3.2" and 6.6 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 1960024100952179840 | 21:59:27.28 +42:08:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:30.86 +42:08:23.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:30.86 +42:08:23.4: 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
Gaia DR3 1960024100952179840,2461185.8473,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 11.95 21:17:51.46 +37:12:27.1
82.66275 -8.44945 galactic Cyg Second-epoch detections are separated by 1.8" and 6.6 pix
The object was found in VSX18" Gaia DR3 1963943000914669952
Type: ROT
# Max. Min./Amp. JD0 Period
15.530 G 15.580 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:51.46 +37:12:27.1: 12.90 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:51.46 +37:12:27.1: 14.25 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 1963943000914669952,2461185.8473,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963943000914669952 20260525.3473 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 25.3473 2461185.8473 12.07 21:13:03.05 +33:40:45.7
79.37583 -10.14794 galactic Cyg Second-epoch detections are separated by 1.3" and 7.0 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 J318.2601+33.6798 | 21:13:03.05 +33:40:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:03.05 +33:40:45.7: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:03.05 +33:40:45.7: 14.32 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.32 +/- 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 J318.2601+33.6798,2461185.8473,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.2601+33.6798 20260525.3473 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 25.3473 2461185.8473 11.88 21:14:26.33 +37:57:13.1
82.73840 -7.44454 galactic Cyg Second-epoch detections are separated by 3.2" and 7.0 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 J318.6237+37.9527 | 21:14:26.33 +37:57:13.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:26.33 +37:57:13.1: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:26.33 +37:57:13.1: 14.13 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 J318.6237+37.9527,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.6237+37.9527 20260525.3473 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 25.3473 2461185.8473 11.73 21:56:29.02 +36:52:32.3
88.19472 -13.93075 galactic Cyg Second-epoch detections are separated by 5.2" and 6.5 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 | 21:56:29.02 +36:52:32.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:29.02 +36:52:32.3: 12.56 +/- 0.13 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:29.02 +36:52:32.3: 14.25 +/- 0.12 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
ATO J329.1195+36.8762,2461185.8473,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 11.97 21:35:23.88 +36:47:17.3
84.88787 -11.21225 galactic Cyg Second-epoch detections are separated by 0.4" and 7.0 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 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:23.88 +36:47:17.3: 12.00 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:23.88 +36:47:17.3: 13.95 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 1951911453183188096,2461185.8473,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.01 21:09:56.53 +42:31:27.0
85.50707 -3.69829 galactic Cyg Second-epoch detections are separated by 5.9" and 5.5 pix
The object was found in VSX 5" ASASSN-V J210956.66+423131.3
Type: SRS
# Max. Min./Amp. JD0 Period
14.950 V 15.130 V 2458004.76000 28.676000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:56.53 +42:31:27.0: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:56.53 +42:31:27.0: 14.44 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.44 +/- 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
ASASSN-V J210956.66+423131.3,2461185.8473,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J210956.66+423131.3 20260525.3473 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 25.3473 2461185.8473 11.91 21:16:52.19 +40:29:56.3
84.92222 -6.03134 galactic Cyg Second-epoch detections are separated by 0.8" and 6.8 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 J319.1926+40.4874 | 21:16:48.73 +40:29:41.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:52.19 +40:29:56.3: 12.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:52.19 +40:29:56.3: 14.44 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 J319.1926+40.4874,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1926+40.4874 20260525.3473 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 25.3473 2461185.8473 12.07 21:17:56.57 +39:27:24.9
84.31058 -6.90243 galactic Cyg Second-epoch detections are separated by 1.3" and 6.5 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 J319.4856+39.4573 | 21:17:59.83 +39:27:20.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.708+/-0.051 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:56.57 +39:27:24.9: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:56.57 +39:27:24.9: 14.46 +/- 0.19 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
ATO J319.4856+39.4573,2461185.8473,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.4856+39.4573 20260525.3473 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 25.3473 2461185.8473 12.10 22:24:31.98 +41:49:20.1
95.69721 -13.15132 galactic Lac Second-epoch detections are separated by 2.6" and 7.3 pix
The object was found in VSX21" ZTF J222433.47+414907.9
Type: EW
# Max. Min./Amp. JD0 Period
18.832 r Y 0.737 r 2458300.91380 0.241391800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:31.98 +41:49:20.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:31.98 +41:49:20.1: 15.15 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.15 +/- 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
ZTF J222433.47+414907.9,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J222433.47+414907.9 20260525.3473 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 25.3473 2461185.8473 11.82 21:27:31.59 +35:50:08.1
83.05169 -10.79637 galactic Cyg Second-epoch detections are separated by 2.0" and 7.2 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 J321.8866+35.8349 | 21:27:31.59 +35:50:08.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:31.59 +35:50:08.1: 12.07 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:31.59 +35:50:08.1: 14.14 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J321.8866+35.8349,2461185.8473,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.8866+35.8349 20260525.3473 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 25.3473 2461185.8473 11.96 21:18:36.52 +38:08:19.0
83.44493 -7.91133 galactic Cyg Second-epoch detections are separated by 3.6" and 7.0 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 | 21:18:36.52 +38:08:19.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:36.52 +38:08:19.0: 12.35 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:36.52 +38:08:19.0: 14.33 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.42 +/- 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,2461185.8473,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.02 21:20:37.24 +41:57:32.3
86.46774 -5.51713 galactic Cyg Second-epoch detections are separated by 0.8" and 6.5 pix
The object was found in VSX 9" Gaia DR3 1968837167691026304
Type: VAR
# Max. Min./Amp. JD0 Period
14.730 G 15.230 G 0.249859000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:37.24 +41:57:32.3: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:37.24 +41:57:32.3: 14.57 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.57 +/- 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 1968837167691026304,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1968837167691026304 20260525.3473 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 25.3473 2461185.8473 11.99 21:20:50.00 +33:44:17.2
80.54651 -11.28806 galactic Cyg Second-epoch detections are separated by 3.6" and 7.2 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 | 21:20:50.00 +33:44:17.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:50.00 +33:44:17.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:50.00 +33:44:17.2: 14.40 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.40 +/- 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,2461185.8473,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.94 21:11:16.17 +36:08:41.0
80.96613 -8.21225 galactic Cyg Second-epoch detections are separated by 2.1" and 6.6 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 | 21:11:16.17 +36:08:41.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:16.17 +36:08:41.0: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:16.17 +36:08:41.0: 14.38 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461185.8473,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:20:39.63 +40:14:13.6
85.23995 -6.73147 galactic Cyg Second-epoch detections are separated by 3.0" and 6.9 pix
The object was found in VSX 1" ZTF J212039.66+401414.9
Type: SR
# Max. Min./Amp. JD0 Period
14.192 r Y 0.357 r 2458387.08510 199.072141700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:39.63 +40:14:13.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:39.63 +40:14:13.6: 14.86 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.86 +/- 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
ZTF J212039.66+401414.9,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212039.66+401414.9 20260525.3473 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 25.3473 2461185.8473 11.81 21:46:08.61 +35:33:30.2
85.68084 -13.58171 galactic Cyg Second-epoch detections are separated by 1.1" and 7.0 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 | 21:46:08.61 +35:33:30.2 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:08.61 +35:33:30.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:08.61 +35:33:30.2: 14.41 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.41 +/- 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,2461185.8473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.91 22:26:27.62 +39:49:37.8
94.88987 -15.02218 galactic Lac Second-epoch detections are separated by 1.6" and 7.5 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 | 22:26:27.62 +39:49:37.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:27.62 +39:49:37.8: 12.98 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:27.62 +39:49:37.8: 15.16 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.93 21:51:38.10 +43:02:19.3
91.45089 -8.57785 galactic Cyg Second-epoch detections are separated by 4.3" and 7.3 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 1960741085614579200 | 21:51:37.65 +43:03:00.3 (Gaia DR3) | DSCT/GDOR (local) | F (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:38.10 +43:02:19.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:38.10 +43:02:19.3: 14.39 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.39 +/- 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 1960741085614579200,2461185.8473,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1960741085614579200 20260525.3473 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 25.3473 2461185.8473 12.12 21:14:10.79 +37:29:35.0
82.36432 -7.72250 galactic Cyg Second-epoch detections are separated by 1.0" and 7.0 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 J318.5432+37.4908 | 21:14:10.79 +37:29:35.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:10.79 +37:29:35.0: 12.77 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:10.79 +37:29:35.0: 14.48 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 J318.5432+37.4908,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.5432+37.4908 20260525.3473 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 25.3473 2461185.8473 12.05 21:18:30.94 +37:37:00.6
83.05263 -8.26023 galactic Cyg Second-epoch detections are separated by 7.2" and 8.1 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 J319.6276+37.6180 | 21:18:30.94 +37:37:00.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:30.94 +37:37:00.6: 12.95 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:30.94 +37:37:00.6: 14.96 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.88 +/- 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
ATO J319.6276+37.6180,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.6276+37.6180 20260525.3473 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 25.3473 2461185.8473 11.88 21:27:39.99 +41:28:15.9
87.06209 -6.78899 galactic Cyg Second-epoch detections are separated by 4.3" and 6.0 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 J321.9194+41.4735 | 21:27:39.99 +41:28:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.496+/-0.057 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:39.99 +41:28:15.9: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:39.99 +41:28:15.9: 14.26 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.26 +/- 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 J321.9194+41.4735,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.9194+41.4735 20260525.3473 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 25.3473 2461185.8473 12.14 21:15:31.87 +39:38:45.3
84.12408 -6.43604 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 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 | 21:15:31.87 +39:38:45.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:31.87 +39:38:45.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:31.87 +39:38:45.3: 14.31 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.31 +/- 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,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.97 21:22:07.42 +37:28:58.6
83.45993 -8.86613 galactic Cyg Second-epoch detections are separated by 0.7" and 6.9 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 | 21:22:07.42 +37:28:58.6 (user input) | T | P | (position from user input) J-Ks=0.542+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:07.42 +37:28:58.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:07.42 +37:28:58.6: 14.37 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.37 +/- 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,2461185.8473,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.88 21:13:30.27 +36:57:14.1
81.87407 -7.99248 galactic Cyg Second-epoch detections are separated by 1.7" and 6.8 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 J318.3624+36.9574 | 21:13:27.61 +36:57:10.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:30.27 +36:57:14.1: 12.38 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:30.27 +36:57:14.1: 14.31 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 J318.3624+36.9574,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.3624+36.9574 20260525.3473 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 25.3473 2461185.8473 12.19 21:22:15.36 +39:25:45.8
84.87767 -7.51696 galactic Cyg Second-epoch detections are separated by 2.9" and 7.3 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 | 21:22:15.36 +39:25:45.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:15.36 +39:25:45.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:15.36 +39:25:45.8: 14.86 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.86 +/- 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.01 21:12:30.88 +37:03:07.0
81.81072 -7.78099 galactic Cyg Second-epoch detections are separated by 3.2" and 7.3 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 1868649805606282624 | 21:12:30.88 +37:03:07.0 (user input) | ROT (local) | K (local) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:30.88 +37:03:07.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:30.88 +37:03:07.0: 14.32 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.32 +/- 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 1868649805606282624,2461185.8473,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1868649805606282624 20260525.3473 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 25.3473 2461185.8473 11.95 21:17:08.35 +38:25:40.4
83.45371 -7.50296 galactic Cyg Second-epoch detections are separated by 1.9" and 7.1 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 | 21:17:08.35 +38:25:40.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:08.35 +38:25:40.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:08.35 +38:25:40.4: 14.25 +/- 0.15 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
target,2461185.8473,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.89 21:15:47.29 +35:00:36.1
80.75631 -9.65747 galactic Cyg Second-epoch detections are separated by 2.4" and 7.4 pix
The object was found in VSX21" ZTF J211547.58+350015.0
Type: EW
# Max. Min./Amp. JD0 Period
18.442 g Y 0.563 g 2458663.92880 0.314042800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:47.29 +35:00:36.1: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:47.29 +35:00:36.1: 14.45 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.45 +/- 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
ZTF J211547.58+350015.0,2461185.8473,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J211547.58+350015.0 20260525.3473 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 25.3473 2461185.8473 12.12 21:30:06.71 +42:42:51.2
88.25795 -6.20639 galactic Cyg Second-epoch detections are separated by 2.3" and 6.3 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 J322.5240+42.7121 | 21:30:06.71 +42:42:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.065+/-0.028 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:06.71 +42:42:51.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:06.71 +42:42:51.2: 14.33 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 J322.5240+42.7121,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.5240+42.7121 20260525.3473 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 25.3473 2461185.8473 12.11 21:09:14.84 +39:51:13.5
83.44791 -5.41151 galactic Cyg Second-epoch detections are separated by 1.9" and 6.9 pix
The object was found in VSX10" Gaia DR3 1968366989030144384
Type: RS
# Max. Min./Amp. JD0 Period
16.710 G 16.850 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:14.84 +39:51:13.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:14.84 +39:51:13.5: 14.31 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.31 +/- 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 1968366989030144384,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1968366989030144384 20260525.3473 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 25.3473 2461185.8473 12.10 21:39:31.73 +40:39:06.9
88.14688 -8.91398 galactic Cyg Second-epoch detections are separated by 1.1" and 6.8 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 J324.8818+40.6426 | 21:39:31.73 +40:39:06.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:31.73 +40:39:06.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:31.73 +40:39:06.9: 14.35 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.35 +/- 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 J324.8818+40.6426,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.8818+40.6426 20260525.3473 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 25.3473 2461185.8473 11.90 21:21:45.46 +38:51:10.6
84.39548 -7.85354 galactic Cyg Second-epoch detections are separated by 5.4" and 7.6 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 | 21:21:45.46 +38:51:10.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:45.46 +38:51:10.6: 12.70 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:45.46 +38:51:10.6: 14.30 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461185.8473,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:14:16.84 +37:13:45.6
82.18395 -7.91748 galactic Cyg Second-epoch detections are separated by 1.8" and 6.7 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 J318.5690+37.2295 | 21:14:16.84 +37:13:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:16.84 +37:13:45.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:16.84 +37:13:45.6: 14.28 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 J318.5690+37.2295,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.5690+37.2295 20260525.3473 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 25.3473 2461185.8473 11.85 21:52:14.88 +36:58:29.7
87.59016 -13.31331 galactic Cyg Second-epoch detections are separated by 3.1" and 7.6 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 | 21:52:14.88 +36:58:29.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.861+/-0.028 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:14.88 +36:58:29.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:14.88 +36:58:29.7: 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
target,2461185.8473,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.09 21:19:39.17 +33:52:22.4
80.47297 -11.01770 galactic Cyg Second-epoch detections are separated by 4.1" and 7.6 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 | 21:19:39.17 +33:52:22.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:39.17 +33:52:22.4: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:39.17 +33:52:22.4: 14.43 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.96 21:14:59.61 +35:56:28.9
81.33280 -8.90258 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 J318.7345+35.9359 | 21:14:59.61 +35:56:28.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:59.61 +35:56:28.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:59.61 +35:56:28.9: 14.33 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.33 +/- 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 J318.7345+35.9359,2461185.8473,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.7345+35.9359 20260525.3473 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 25.3473 2461185.8473 12.10 22:02:22.40 +41:34:46.0
92.10471 -10.95581 galactic Lac Second-epoch detections are separated by 0.5" and 7.1 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 | 22:02:22.40 +41:34:46.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:22.40 +41:34:46.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:22.40 +41:34:46.0: 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
target,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.05 21:15:38.33 +36:40:31.9
81.96407 -8.49452 galactic Cyg Second-epoch detections are separated by 3.0" and 7.4 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 J318.9104+36.6744 | 21:15:38.33 +36:40:31.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:38.33 +36:40:31.9: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:38.33 +36:40:31.9: 14.69 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.69 +/- 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 J318.9104+36.6744,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.9104+36.6744 20260525.3473 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 25.3473 2461185.8473 12.01 21:18:56.28 +38:50:10.9
83.99624 -7.47256 galactic Cyg Second-epoch detections are separated by 2.1" and 7.1 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 J319.7340+38.8370 | 21:18:56.28 +38:50:10.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:56.28 +38:50:10.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:56.28 +38:50:10.9: 14.67 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.67 +/- 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 J319.7340+38.8370,2461185.8473,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.7340+38.8370 20260525.3473 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 25.3473 2461185.8473 12.05 21:29:27.20 +34:33:19.8
82.41941 -11.98355 galactic Cyg Second-epoch detections are separated by 2.0" and 7.2 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 | 21:29:27.20 +34:33:19.8 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:27.20 +34:33:19.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:27.20 +34:33:19.8: 14.87 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.87 +/- 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,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:17:06.68 +41:12:00.4
85.46159 -5.57777 galactic Cyg Second-epoch detections are separated by 5.4" and 5.8 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 J319.2791+41.1991 | 21:17:06.68 +41:12:00.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:06.68 +41:12:00.4: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:06.68 +41:12:00.4: 14.31 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.31 +/- 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 J319.2791+41.1991,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.2791+41.1991 20260525.3473 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 25.3473 2461185.8473 12.04 21:35:28.32 +41:43:14.3
88.30391 -7.60994 galactic Cyg Second-epoch detections are separated by 0.5" and 6.7 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 | 21:35:28.32 +41:43:14.3 (user input) | T | P | (position from user input) J-Ks=0.797+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:28.32 +41:43:14.3: 12.28 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:28.32 +41:43:14.3: 14.52 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.09 +/- 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
target,2461185.8473,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.91 21:20:53.12 +35:23:53.9
81.77067 -10.14366 galactic Cyg Second-epoch detections are separated by 2.3" and 6.7 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 J320.2294+35.4005 | 21:20:53.12 +35:23:53.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.223+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:53.12 +35:23:53.9: 13.31 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:53.12 +35:23:53.9: 14.43 +/- 0.17 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 J320.2294+35.4005,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.2294+35.4005 20260525.3473 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 25.3473 2461185.8473 12.20 21:28:05.33 +38:26:58.1
84.99355 -9.01142 galactic Cyg Second-epoch detections are separated by 1.0" and 6.8 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 | 21:28:05.33 +38:26:58.1 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:05.33 +38:26:58.1: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:05.33 +38:26:58.1: 14.47 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.47 +/- 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,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.11 21:21:50.20 +36:52:22.5
82.97850 -9.25262 galactic Cyg Second-epoch detections are separated by 1.8" and 7.1 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 J320.4600+36.8641 | 21:21:50.20 +36:52:22.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:50.20 +36:52:22.5: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:50.20 +36:52:22.5: 14.31 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.31 +/- 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 J320.4600+36.8641,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.4600+36.8641 20260525.3473 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 25.3473 2461185.8473 11.96 21:15:26.44 +37:30:51.4
82.55291 -7.89005 galactic Cyg Second-epoch detections are separated by 1.6" and 6.9 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 J318.8598+37.5136 | 21:15:26.44 +37:30:51.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.597+/-0.117 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:26.44 +37:30:51.4: 12.25 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:26.44 +37:30:51.4: 14.06 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 J318.8598+37.5136,2461185.8473,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.8598+37.5136 20260525.3473 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 25.3473 2461185.8473 12.04 21:22:02.49 +35:07:47.2
81.74186 -10.50003 galactic Cyg Second-epoch detections are separated by 1.9" and 7.3 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 | 21:22:02.49 +35:07:47.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:02.49 +35:07:47.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:02.49 +35:07:47.2: 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,2461185.8473,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.18 21:22:02.31 +40:43:48.2
85.77833 -6.57119 galactic Cyg Second-epoch detections are separated by 1.0" and 6.7 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 | 21:22:02.31 +40:43:48.2 (user input) | T | P | (position from user input) J-Ks=0.832+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:02.31 +40:43:48.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:02.31 +40:43:48.2: 14.46 +/- 0.18 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
target,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.08 21:17:11.05 +36:26:19.7
82.00604 -8.88261 galactic Cyg Second-epoch detections are separated by 1.4" and 7.0 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 J319.3030+36.4286 | 21:17:11.05 +36:26:19.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.337+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:11.05 +36:26:19.7: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:11.05 +36:26:19.7: 14.44 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 J319.3030+36.4286,2461185.8473,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3030+36.4286 20260525.3473 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 25.3473 2461185.8473 12.11 21:24:04.31 +39:44:04.0
85.34476 -7.54930 galactic Cyg Second-epoch detections are separated by 1.7" and 7.0 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 | 21:24:04.31 +39:44:04.0 (user input) | T | P | (position from user input) J-Ks=0.801+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:04.31 +39:44:04.0: 12.55 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:04.31 +39:44:04.0: 14.23 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.91 21:11:19.09 +37:30:42.3
81.98834 -7.29410 galactic Cyg Second-epoch detections are separated by 1.5" and 7.0 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 J317.8268+37.5139 | 21:11:19.09 +37:30:42.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:19.09 +37:30:42.3: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:19.09 +37:30:42.3: 14.30 +/- 0.17 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
ATO J317.8268+37.5139,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.8268+37.5139 20260525.3473 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 25.3473 2461185.8473 12.20 21:09:57.15 +38:42:12.3
82.68845 -6.28964 galactic Cyg Second-epoch detections are separated by 8.0" and 5.4 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 J317.4891+38.7050 | 21:09:57.15 +38:42:12.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:57.15 +38:42:12.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:57.15 +38:42:12.3: 14.86 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.86 +/- 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 J317.4891+38.7050,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.4891+38.7050 20260525.3473 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 25.3473 2461185.8473 11.90 21:33:38.40 +34:07:28.0
82.74522 -12.89540 galactic Cyg Second-epoch detections are separated by 0.7" and 7.2 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 | 21:33:38.40 +34:07:28.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:38.40 +34:07:28.0: 13.00 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:38.40 +34:07:28.0: 14.83 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461185.8473,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.88 21:24:44.61 +34:18:56.5
81.54501 -11.46627 galactic Cyg Second-epoch detections are separated by 5.0" and 7.6 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 J321.1853+34.3173 | 21:24:44.61 +34:18:56.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:44.61 +34:18:56.5: 12.37 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:44.61 +34:18:56.5: 14.36 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 J321.1853+34.3173,2461185.8473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.1853+34.3173 20260525.3473 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 25.3473 2461185.8473 12.14 21:23:30.98 +34:11:51.6
81.27788 -11.36794 galactic Cyg Second-epoch detections are separated by 7.0" and 6.7 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 J320.8931+34.1927 | 21:23:30.98 +34:11:51.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:30.98 +34:11:51.6: 12.99 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:30.98 +34:11:51.6: 14.40 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 J320.8931+34.1927,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.8931+34.1927 20260525.3473 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 25.3473 2461185.8473 12.12 21:15:36.01 +39:45:24.1
84.21402 -6.36927 galactic Cyg Second-epoch detections are separated by 0.5" and 6.6 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 | 21:15:36.01 +39:45:24.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:36.01 +39:45:24.1: 12.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:36.01 +39:45:24.1: 14.28 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.02 21:20:26.81 +34:06:13.7
80.75886 -10.97701 galactic Cyg Second-epoch detections are separated by 1.2" and 7.0 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 | 21:20:26.81 +34:06:13.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:26.81 +34:06:13.7: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:26.81 +34:06:13.7: 14.52 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.52 +/- 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,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:09:54.44 +40:43:36.8
84.17882 -4.91320 galactic Cyg Second-epoch detections are separated by 1.3" and 6.5 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 | 21:09:54.44 +40:43:36.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:54.44 +40:43:36.8: 12.49 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:54.44 +40:43:36.8: 14.54 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.15 21:14:16.57 +40:58:14.5
84.92411 -5.35023 galactic Cyg Second-epoch detections are separated by 2.6" and 6.3 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 | 21:14:16.57 +40:58:14.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:16.57 +40:58:14.5: 12.64 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:16.57 +40:58:14.5: 14.57 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.99 22:06:26.75 +38:35:58.2
90.88697 -13.79692 galactic Lac Second-epoch detections are separated by 0.8" and 6.8 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 | 22:06:26.75 +38:35:58.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:26.75 +38:35:58.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:26.75 +38:35:58.2: 14.90 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.90 +/- 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,2461185.8473,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.01 21:11:55.95 +39:55:31.5
83.85205 -5.74113 galactic Cyg Second-epoch detections are separated by 2.4" and 6.7 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 | 21:11:55.95 +39:55:31.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:55.95 +39:55:31.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:55.95 +39:55:31.5: 14.12 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461185.8473,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.07 21:27:06.47 +33:44:08.5
81.47623 -12.22248 galactic Cyg Second-epoch detections are separated by 2.6" and 7.0 pix
The object was found in VSX 7" 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:06.47 +33:44:08.5: 12.79 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:06.47 +33:44:08.5: 14.65 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 1854317224858662912,2461185.8473,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 11.89 21:21:25.57 +36:56:48.2
82.97382 -9.14236 galactic Cyg Second-epoch detections are separated by 1.1" and 6.9 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 1963888609447842432 | 21:21:23.43 +36:56:11.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:25.57 +36:56:48.2: 12.55 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:25.57 +36:56:48.2: 14.12 +/- 0.13 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
Gaia DR3 1963888609447842432,2461185.8473,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963888609447842432 20260525.3473 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 25.3473 2461185.8473 12.09 21:24:48.14 +42:23:48.8
87.32957 -5.75451 galactic Cyg Second-epoch detections are separated by 2.1" and 6.7 pix
The object was found in VSX 7" Gaia DR3 1970362911872143488
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.180 G 15.210 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:48.14 +42:23:48.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:48.14 +42:23:48.8: 14.47 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.47 +/- 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 1970362911872143488,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1970362911872143488 20260525.3473 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 25.3473 2461185.8473 12.25 21:13:14.13 +42:38:33.7
86.00886 -4.06009 galactic Cyg Second-epoch detections are separated by 3.2" and 6.1 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 J318.3136+42.6446 | 21:13:14.13 +42:38:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:14.13 +42:38:33.7: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:14.13 +42:38:33.7: 14.77 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.77 +/- 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 J318.3136+42.6446,2461185.8473,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.3136+42.6446 20260525.3473 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 25.3473 2461185.8473 12.10 21:16:57.10 +42:07:19.2
86.10677 -4.91596 galactic Cyg Second-epoch detections are separated by 0.7" and 6.7 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 J319.2347+42.1229 | 21:16:57.10 +42:07:19.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:57.10 +42:07:19.2: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:57.10 +42:07:19.2: 14.22 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.22 +/- 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 J319.2347+42.1229,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.2347+42.1229 20260525.3473 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 25.3473 2461185.8473 12.11 21:16:51.29 +37:38:57.4
82.84651 -8.00034 galactic Cyg Second-epoch detections are separated by 2.2" and 6.5 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 | 21:16:51.29 +37:38:57.4 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:51.29 +37:38:57.4: 12.91 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:51.29 +37:38:57.4: 14.66 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:08:48.24 +42:15:28.4
85.16814 -3.72431 galactic Cyg Second-epoch detections are separated by 0.5" and 6.6 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 | 21:08:48.24 +42:15:28.4 (user input) | T | P | (position from user input) J-Ks=0.565+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:08:48.24 +42:15:28.4: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:08:48.24 +42:15:28.4: 14.60 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.60 +/- 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,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.94 22:15:17.88 +37:28:35.3
91.64889 -15.73497 galactic Lac Second-epoch detections are separated by 1.4" and 7.5 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 | 22:15:17.88 +37:28:35.3 (user input) | T | P | (position from user input) J-Ks=0.804+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:15:17.88 +37:28:35.3: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:15:17.88 +37:28:35.3: 15.24 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.24 +/- 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,2461185.8473,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.04 21:26:55.09 +38:03:54.1
84.55480 -9.12495 galactic Cyg Second-epoch detections are separated by 2.1" and 6.5 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 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)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:55.09 +38:03:54.1: 13.23 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:55.09 +38:03:54.1: 14.45 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.18 +/- 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
Large-amplitude variable Gaia DR2 1964230213966061824,2461185.8473,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.08 21:19:14.73 +35:22:02.5
81.51259 -9.92436 galactic Cyg Second-epoch detections are separated by 2.0" and 7.0 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 | 21:19:14.73 +35:22:02.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:14.73 +35:22:02.5: 13.08 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:14.73 +35:22:02.5: 14.56 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461185.8473,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.02 21:32:06.88 +39:41:52.2
86.43925 -8.65355 galactic Cyg Second-epoch detections are separated by 1.6" and 6.7 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 | 21:32:06.88 +39:41:52.2 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:06.88 +39:41:52.2: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:06.88 +39:41:52.2: 14.35 +/- 0.14 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
target,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.20 21:09:05.11 +42:36:25.8
85.46092 -3.52604 galactic Cyg Second-epoch detections are separated by 3.4" and 7.1 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 | 21:09:05.11 +42:36:25.8 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:05.11 +42:36:25.8: 12.44 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:05.11 +42:36:25.8: 14.50 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.35 +/- 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
target,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.02 21:13:06.79 +36:56:00.8
81.80522 -7.94912 galactic Cyg Second-epoch detections are separated by 2.0" and 7.1 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 | 21:13:06.79 +36:56:00.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:06.79 +36:56:00.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:06.79 +36:56:00.8: 14.41 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.41 +/- 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,2461185.8473,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.20 21:28:11.68 +40:25:03.1
86.39523 -7.61496 galactic Cyg Second-epoch detections are separated by 0.3" and 6.7 pix
The object was found in VSX 2" ASASSN-V J212811.82+402504.6
Type: SRS
# Max. Min./Amp. JD0 Period
15.040 V 15.180 V 2457303.88500 24.219000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:11.68 +40:25:03.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:11.68 +40:25:03.1: 14.57 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.57 +/- 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
ASASSN-V J212811.82+402504.6,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212811.82+402504.6 20260525.3473 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 25.3473 2461185.8473 11.95 21:12:33.74 +36:07:03.1
81.12460 -8.42272 galactic Cyg Second-epoch detections are separated by 4.7" and 6.5 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 J318.1412+36.1204 | 21:12:33.74 +36:07:03.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.406+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:33.74 +36:07:03.1: 12.05 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:33.74 +36:07:03.1: 14.30 +/- 0.17 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 J318.1412+36.1204,2461185.8473,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.1412+36.1204 20260525.3473 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 25.3473 2461185.8473 12.21 21:23:28.72 +41:52:46.5
86.78849 -5.94968 galactic Cyg Second-epoch detections are separated by 0.5" and 6.7 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 | 21:23:28.72 +41:52:46.5 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:28.72 +41:52:46.5: 12.59 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:28.72 +41:52:46.5: 14.71 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.13 21:14:16.35 +39:30:16.2
83.85290 -6.35730 galactic Cyg Second-epoch detections are separated by 0.9" and 6.7 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 | 21:14:16.35 +39:30:16.2 (user input) | T | P | (position from user input) J-Ks=0.766+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:16.35 +39:30:16.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:16.35 +39:30:16.2: 14.73 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.73 +/- 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,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:13:36.47 +40:33:16.4
84.53300 -5.54413 galactic Cyg Second-epoch detections are separated by 1.0" and 6.8 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 J318.4005+40.5539 | 21:13:36.47 +40:33:16.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.729+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:36.47 +40:33:16.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:36.47 +40:33:16.4: 14.21 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 J318.4005+40.5539,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.4005+40.5539 20260525.3473 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 25.3473 2461185.8473 12.12 21:28:24.99 +39:10:02.1
85.54663 -8.54185 galactic Cyg Second-epoch detections are separated by 0.5" and 6.9 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 | 21:28:24.99 +39:10:02.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:24.99 +39:10:02.1: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:24.99 +39:10:02.1: 14.73 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.73 +/- 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,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:16:01.67 +41:46:07.3
85.73171 -5.03728 galactic Cyg Second-epoch detections are separated by 1.7" and 6.4 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 J319.0030+41.7706 | 21:16:01.67 +41:46:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:01.67 +41:46:07.3: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:01.67 +41:46:07.3: 14.45 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 J319.0030+41.7706,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.0030+41.7706 20260525.3473 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 25.3473 2461185.8473 12.09 21:26:05.34 +35:06:07.9
82.31316 -11.10908 galactic Cyg Second-epoch detections are separated by 1.6" and 7.0 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 | 21:26:05.34 +35:06:07.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:05.34 +35:06:07.9: 12.73 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:05.34 +35:06:07.9: 14.84 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.58 +/- 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
target,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.15 21:12:30.57 +39:48:04.7
83.83678 -5.90676 galactic Cyg Second-epoch detections are separated by 2.6" and 7.1 pix
The object was found in VSX 5" ZTF J211230.68+394809.7
Type: EW
# Max. Min./Amp. JD0 Period
14.405 r Y 0.722 r 2458475.63270 0.317594200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:30.57 +39:48:04.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:30.57 +39:48:04.7: 14.50 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.50 +/- 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 J211230.68+394809.7,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J211230.68+394809.7 20260525.3473 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 25.3473 2461185.8473 12.07 21:12:21.74 +39:39:54.0
83.71722 -5.97913 galactic Cyg Second-epoch detections are separated by 2.7" and 6.2 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 | 21:12:21.74 +39:39:54.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:21.74 +39:39:54.0: 13.09 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:21.74 +39:39:54.0: 14.56 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461185.8473,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.17 21:13:03.49 +36:09:05.9
81.21865 -8.47302 galactic Cyg Second-epoch detections are separated by 3.8" and 7.6 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 | 21:13:03.49 +36:09:05.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:03.49 +36:09:05.9: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:03.49 +36:09:05.9: 14.56 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.56 +/- 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,2461185.8473,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.12 21:22:43.62 +37:39:17.5
83.66878 -8.83059 galactic Cyg Second-epoch detections are separated by 2.1" and 7.1 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 | 21:22:43.62 +37:39:17.5 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:43.62 +37:39:17.5: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:43.62 +37:39:17.5: 14.22 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.13 21:09:38.79 +38:16:13.8
82.32655 -6.53796 galactic Cyg Second-epoch detections are separated by 1.4" and 7.0 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 | 21:09:38.79 +38:16:13.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:38.79 +38:16:13.8: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:38.79 +38:16:13.8: 14.22 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:26:10.16 +38:57:59.5
85.08957 -8.38011 galactic Cyg Second-epoch detections are separated by 5.3" and 7.7 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 | 21:26:10.16 +38:57:59.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:10.16 +38:57:59.5: 13.08 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:10.16 +38:57:59.5: 15.02 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.03 21:36:18.16 +40:03:04.6
87.27748 -8.94400 galactic Cyg Second-epoch detections are separated by 1.6" and 6.9 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 J324.0798+40.0481 | 21:36:17.72 +40:02:25.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:18.16 +40:03:04.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:18.16 +40:03:04.6: 14.03 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 J324.0798+40.0481,2461185.8473,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.0798+40.0481 20260525.3473 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 25.3473 2461185.8473 12.06 21:15:44.18 +40:24:58.2
84.71210 -5.93297 galactic Cyg Second-epoch detections are separated by 0.2" and 6.6 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 | 21:15:44.18 +40:24:58.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:44.18 +40:24:58.2: 12.99 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:44.18 +40:24:58.2: 14.47 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461185.8473,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.97 21:50:34.17 +37:11:04.4
87.46696 -12.93698 galactic Cyg Second-epoch detections are separated by 3.9" and 7.2 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 | 21:50:34.17 +37:11:04.4 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:34.17 +37:11:04.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:34.17 +37:11:04.4: 14.54 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.54 +/- 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,2461185.8473,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.21 21:31:39.14 +36:46:27.5
84.32457 -10.70545 galactic Cyg Second-epoch detections are separated by 1.5" and 6.8 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 | 21:31:39.14 +36:46:27.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:39.14 +36:46:27.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:39.14 +36:46:27.5: 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,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.06 21:24:33.16 +35:18:35.4
82.23804 -10.74007 galactic Cyg Second-epoch detections are separated by 4.4" and 6.7 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 | 21:24:33.16 +35:18:35.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:33.16 +35:18:35.4: 12.66 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:33.16 +35:18:35.4: 14.65 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461185.8473,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.09 21:12:13.58 +35:59:01.3
80.97860 -8.46358 galactic Cyg Second-epoch detections are separated by 2.7" and 6.6 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 | 21:12:13.58 +35:59:01.3 (user input) | T | P | (position from user input) J-Ks=0.669+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:13.58 +35:59:01.3: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:13.58 +35:59:01.3: 14.23 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.23 +/- 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,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.20 21:29:06.42 +42:10:44.9
87.75128 -6.46542 galactic Cyg Second-epoch detections are separated by 3.2" and 6.2 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 J322.2786+42.1706 | 21:29:06.42 +42:10:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.372+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:06.42 +42:10:44.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:06.42 +42:10:44.9: 14.48 +/- 0.17 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
ATO J322.2786+42.1706,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.2786+42.1706 20260525.3473 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 25.3473 2461185.8473 12.07 21:21:51.44 +35:01:42.5
81.64127 -10.54364 galactic Cyg Second-epoch detections are separated by 1.5" and 6.8 pix
The object was found in VSX11" Gaia DR3 1855428899833377792
Type: VAR
# Max. Min./Amp. JD0 Period
15.190 G 15.200 G 0.086773500000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:51.44 +35:01:42.5: 12.74 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:51.44 +35:01:42.5: 14.30 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 1855428899833377792,2461185.8473,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1855428899833377792 20260525.3473 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 25.3473 2461185.8473 12.19 21:17:00.50 +40:40:07.8
85.06361 -5.93250 galactic Cyg Second-epoch detections are separated by 4.2" and 6.0 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 J319.2612+40.6623 | 21:17:00.50 +40:40:07.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:00.50 +40:40:07.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:00.50 +40:40:07.8: 14.29 +/- 0.14 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
ATO J319.2612+40.6623,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.2612+40.6623 20260525.3473 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 25.3473 2461185.8473 11.91 21:43:03.17 +37:32:30.3
86.55464 -11.68646 galactic Cyg Second-epoch detections are separated by 0.5" and 7.0 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 | 21:43:03.17 +37:32:30.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:03.17 +37:32:30.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:03.17 +37:32:30.3: 14.31 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.31 +/- 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,2461185.8473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.15 21:16:45.31 +37:40:26.8
82.85092 -7.96893 galactic Cyg Second-epoch detections are separated by 1.1" and 6.9 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 J319.1791+37.6788 | 21:16:45.31 +37:40:26.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:45.31 +37:40:26.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:45.31 +37:40:26.8: 14.70 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.70 +/- 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 J319.1791+37.6788,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1791+37.6788 20260525.3473 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 25.3473 2461185.8473 12.18 21:20:36.52 +39:47:04.5
84.90789 -7.04164 galactic Cyg Second-epoch detections are separated by 4.7" and 6.2 pix
The object was found in VSX25" Gaia DR3 1965551036670131456
Type: VAR
# Max. Min./Amp. JD0 Period
16.430 G 16.450 G 0.034394400000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:36.52 +39:47:04.5: 12.77 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:36.52 +39:47:04.5: 14.34 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 1965551036670131456,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1965551036670131456 20260525.3473 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 25.3473 2461185.8473 12.24 21:23:22.12 +39:56:38.4
85.39775 -7.30563 galactic Cyg Second-epoch detections are separated by 1.1" and 6.9 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 | 21:23:22.12 +39:56:38.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:22.12 +39:56:38.4: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:22.12 +39:56:38.4: 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,2461185.8473,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.10 21:17:14.63 +35:36:37.3
81.40587 -9.46176 galactic Cyg Second-epoch detections are separated by 1.2" and 7.2 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 J319.3109+35.6108 | 21:17:14.63 +35:36:37.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.415+/-0.054 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:14.63 +35:36:37.3: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:14.63 +35:36:37.3: 14.36 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 J319.3109+35.6108,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3109+35.6108 20260525.3473 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 25.3473 2461185.8473 12.09 21:46:00.43 +37:21:18.7
86.87737 -12.21460 galactic Cyg Second-epoch detections are separated by 1.2" and 6.8 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 J326.5116+37.3556 | 21:46:02.57 +37:20:47.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=-0.206+/-0.121 (B)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:00.43 +37:21:18.7: 12.66 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:00.43 +37:21:18.7: 14.17 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 J326.5116+37.3556,2461185.8473,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J326.5116+37.3556 20260525.3473 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 25.3473 2461185.8473 12.05 21:25:09.83 +35:16:05.1
82.29719 -10.85806 galactic Cyg Second-epoch detections are separated by 1.2" and 7.0 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 | 21:25:09.83 +35:16:05.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:09.83 +35:16:05.1: 12.65 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:09.83 +35:16:05.1: 14.56 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.16 21:25:52.28 +34:14:43.9
81.66122 -11.68131 galactic Cyg Second-epoch detections are separated by 2.3" and 7.4 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 | 21:25:52.28 +34:14:43.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:52.28 +34:14:43.9: 12.68 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:52.28 +34:14:43.9: 14.74 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.58 +/- 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,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:28:04.36 +43:01:07.6
88.19820 -5.72803 galactic Cyg Second-epoch detections are separated by 1.9" and 6.3 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 J322.0196+43.0178 | 21:28:04.36 +43:01:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.678+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:04.36 +43:01:07.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:04.36 +43:01:07.6: 14.82 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.82 +/- 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 J322.0196+43.0178,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.0196+43.0178 20260525.3473 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 25.3473 2461185.8473 12.12 21:23:39.86 +36:34:06.7
83.01902 -9.72717 galactic Cyg Second-epoch detections are separated by 2.3" and 7.3 pix
The object was found in VSX 3" Gaia DR3 1963635653053460096
Type: ROT
# Max. Min./Amp. JD0 Period
14.550 G 14.610 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:39.86 +36:34:06.7: 12.87 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:39.86 +36:34:06.7: 14.47 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 1963635653053460096,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1963635653053460096 20260525.3473 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 25.3473 2461185.8473 12.04 21:13:26.53 +37:18:51.3
82.13155 -7.73764 galactic Cyg Second-epoch detections are separated by 3.5" and 6.5 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 J318.3568+37.3153 | 21:13:26.53 +37:18:51.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:26.53 +37:18:51.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:26.53 +37:18:51.3: 15.02 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.02 +/- 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 J318.3568+37.3153,2461185.8473,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.3568+37.3153 20260525.3473 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 25.3473 2461185.8473 12.12 21:19:42.47 +42:04:26.7
86.43055 -5.31557 galactic Cyg Second-epoch detections are separated by 1.0" and 6.6 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 J319.9220+42.0654 | 21:19:42.47 +42:04:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:42.47 +42:04:26.7: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:42.47 +42:04:26.7: 14.38 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.38 +/- 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 J319.9220+42.0654,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.9220+42.0654 20260525.3473 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 25.3473 2461185.8473 12.16 21:48:47.70 +38:52:56.3
88.32169 -11.41829 galactic Cyg Second-epoch detections are separated by 2.7" and 6.6 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 | 21:48:47.70 +38:52:56.3 (user input) | T | P | (position from user input) J-Ks=0.919+/-0.036 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:47.70 +38:52:56.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:47.70 +38:52:56.3: 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,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.15 22:10:15.65 +41:33:59.3
93.30184 -11.84978 galactic Lac Second-epoch detections are separated by 2.7" and 6.7 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 J332.5657+41.5671 | 22:10:15.65 +41:33:59.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:15.65 +41:33:59.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:15.65 +41:33:59.3: 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+41.5671,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.24 22:20:33.29 +42:19:01.7
95.34610 -12.33116 galactic Lac Second-epoch detections are separated by 7.8" and 7.3 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 | 22:20:33.29 +42:19:01.7 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:33.29 +42:19:01.7: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:33.29 +42:19:01.7: 14.55 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.55 +/- 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,2461185.8473,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.13 21:35:21.80 +41:16:18.5
87.98170 -7.92608 galactic Cyg Second-epoch detections are separated by 1.3" and 6.6 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 J323.8437+41.2602 | 21:35:21.80 +41:16:18.5 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.387+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:21.80 +41:16:18.5: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:21.80 +41:16:18.5: 14.58 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.58 +/- 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+41.2602,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.22 21:20:38.41 +41:21:07.4
86.03629 -5.94617 galactic Cyg Second-epoch detections are separated by 1.3" and 6.5 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 | 21:20:38.41 +41:21:07.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:38.41 +41:21:07.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:38.41 +41:21:07.4: 14.50 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.50 +/- 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,2461185.8473,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.12 21:34:17.47 +36:20:30.1
84.41054 -11.38430 galactic Cyg Second-epoch detections are separated by 1.7" and 6.8 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 | 21:34:17.47 +36:20:30.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:17.47 +36:20:30.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:17.47 +36:20:30.1: 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
target,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:19:00.61 +40:46:44.4
85.40859 -6.12818 galactic Cyg Second-epoch detections are separated by 2.8" and 7.1 pix
The object was found in VSX18" ZTF J211859.27+404635.6
Type: RS
# Max. Min./Amp. JD0 Period
18.280 r Y 0.363 r 2458602.03250 5.377356100000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:00.61 +40:46:44.4: 13.21 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:00.61 +40:46:44.4: 14.96 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.29 +/- 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
ZTF J211859.27+404635.6,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J211859.27+404635.6 20260525.3473 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 25.3473 2461185.8473 12.19 21:34:52.89 +37:58:12.8
85.63527 -10.28021 galactic Cyg Second-epoch detections are separated by 3.6" and 7.5 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 J323.7196+37.9673 | 21:34:52.89 +37:58:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.923+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:52.89 +37:58:12.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:52.89 +37:58:12.8: 14.48 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.48 +/- 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 J323.7196+37.9673,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.7196+37.9673 20260525.3473 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 25.3473 2461185.8473 12.19 21:17:18.89 +40:12:48.6
84.77451 -6.29041 galactic Cyg Second-epoch detections are separated by 1.3" and 6.8 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 J319.3208+40.2172 | 21:17:18.89 +40:12:48.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:18.89 +40:12:48.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:18.89 +40:12:48.6: 14.74 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.74 +/- 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 J319.3208+40.2172,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3208+40.2172 20260525.3473 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 25.3473 2461185.8473 12.32 21:21:22.32 +39:19:41.6
84.68398 -7.46658 galactic Cyg Second-epoch detections are separated by 1.7" and 6.7 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 | 21:21:22.32 +39:19:41.6 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:22.32 +39:19:41.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:22.32 +39:19:41.6: 14.66 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.66 +/- 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,2461185.8473,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.06 21:23:41.27 +34:38:47.8
81.63018 -11.07916 galactic Cyg Second-epoch detections are separated by 5.9" and 7.2 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 | 21:23:41.27 +34:38:47.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:41.27 +34:38:47.8: 13.26 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:41.27 +34:38:47.8: 14.33 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461185.8473,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.30 21:22:46.51 +41:12:15.2
86.21510 -6.33495 galactic Cyg Second-epoch detections are separated by 1.7" and 7.0 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 | 21:22:46.51 +41:12:15.2 (user input) | T | P | (position from user input) J-Ks=1.053+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:46.51 +41:12:15.2: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:46.51 +41:12:15.2: 14.55 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.55 +/- 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,2461185.8473,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:14:55.67 +38:15:22.6
83.02701 -7.30698 galactic Cyg Second-epoch detections are separated by 2.8" and 6.7 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 | 21:14:55.67 +38:15:22.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:55.67 +38:15:22.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:55.67 +38:15:22.6: 15.02 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.02 +/- 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:28:49.03 +41:29:04.0
87.22760 -6.92909 galactic Cyg Second-epoch detections are separated by 1.9" and 6.7 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 | 21:28:49.03 +41:29:04.0 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.048 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:49.03 +41:29:04.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:49.03 +41:29:04.0: 14.82 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.82 +/- 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,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.05 22:07:43.00 +39:34:56.3
91.69744 -13.16011 galactic Lac Second-epoch detections are separated by 5.4" and 7.4 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 | Large-amplitude variable Gaia DR2 1956357710708103040 | 22:07:41.75 +39:34:42.0 (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) SpType: G4 (LAMOST DR5) J-Ks=0.644+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:43.00 +39:34:56.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:43.00 +39:34:56.3: 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
Large-amplitude variable Gaia DR2 1956357710708103040,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1956357710708103040 20260525.3473 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 25.3473 2461185.8473 12.13 21:21:50.96 +37:08:26.3
83.17398 -9.06705 galactic Cyg Second-epoch detections are separated by 1.5" and 7.1 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 | 21:21:50.96 +37:08:26.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:50.96 +37:08:26.3: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:50.96 +37:08:26.3: 14.72 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.72 +/- 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,2461185.8473,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.28 21:21:17.06 +40:50:15.1
85.75397 -6.39415 galactic Cyg Second-epoch detections are separated by 1.0" and 6.5 pix
The object was found in VSX 7" Gaia DR3 1965754618120828928
Type: E
# Max. Min./Amp. JD0 Period
17.920 G 18.140 G 0.422508000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:17.06 +40:50:15.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:17.06 +40:50:15.1: 14.77 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.77 +/- 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 1965754618120828928,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1965754618120828928 20260525.3473 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 25.3473 2461185.8473 12.35 21:13:21.93 +42:19:57.4
85.79940 -4.29049 galactic Cyg Second-epoch detections are separated by 0.7" and 6.4 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 J318.3442+42.3357 | 21:13:21.93 +42:19:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.829+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:21.93 +42:19:57.4: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:21.93 +42:19:57.4: 14.63 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.63 +/- 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 J318.3442+42.3357,2461185.8473,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.3442+42.3357 20260525.3473 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 25.3473 2461185.8473 12.12 21:13:50.26 +41:55:52.2
85.56726 -4.62998 galactic Cyg Second-epoch detections are separated by 1.9" and 6.4 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 J318.4573+41.9248 | 21:13:50.26 +41:55:52.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:50.26 +41:55:52.2: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:50.26 +41:55:52.2: 15.12 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.12 +/- 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 J318.4573+41.9248,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.4573+41.9248 20260525.3473 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 25.3473 2461185.8473 12.31 21:26:58.76 +38:06:04.9
84.58930 -9.10751 galactic Cyg Second-epoch detections are separated by 3.7" and 6.3 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 | 21:26:58.76 +38:06:04.9 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.057 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:58.76 +38:06:04.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:58.76 +38:06:04.9: 14.64 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.64 +/- 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.15 21:43:55.49 +42:55:24.1
90.28800 -7.75522 galactic Cyg Second-epoch detections are separated by 3.2" and 6.9 pix
The object was found in VSX 2" V2459 Cyg
Type: M
# Max. Min./Amp. JD0 Period
16.668 g Y 2.265 g 2458275.24720 272.346136800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:55.49 +42:55:24.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:55.49 +42:55:24.1: 15.45 +/- 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
V2459 Cyg,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2459 Cyg 20260525.3473 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 25.3473 2461185.8473 12.05 21:16:40.26 +38:16:21.7
83.27658 -7.54385 galactic Cyg Second-epoch detections are separated by 2.7" and 7.2 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 J319.1530+38.2691 | 21:16:40.26 +38:16:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:40.26 +38:16:21.7: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:40.26 +38:16:21.7: 14.52 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.52 +/- 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 J319.1530+38.2691,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1530+38.2691 20260525.3473 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 25.3473 2461185.8473 12.17 21:31:28.06 +39:47:03.7
86.40829 -8.50516 galactic Cyg Second-epoch detections are separated by 2.1" and 6.8 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 | 21:31:28.06 +39:47:03.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:28.06 +39:47:03.7: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:28.06 +39:47:03.7: 15.02 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.02 +/- 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,2461185.8473,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.04 21:42:31.17 +35:51:15.0
85.31964 -12.87102 galactic Cyg Second-epoch detections are separated by 1.1" and 7.1 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 J325.6327+35.8537 | 21:42:31.17 +35:51:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:31.17 +35:51:15.0: 13.34 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:31.17 +35:51:15.0: 14.66 +/- 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+35.8537,2461185.8473,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.16 21:43:09.61 +39:56:52.7
88.19604 -9.90016 galactic Cyg Second-epoch detections are separated by 1.4" and 6.9 pix
The object was found in VSX13" Gaia DR3 1954296951040334464
Type: ROT
# Max. Min./Amp. JD0 Period
15.750 G 15.780 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:09.61 +39:56:52.7: 13.26 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:09.61 +39:56:52.7: 14.42 +/- 0.13 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
Gaia DR3 1954296951040334464,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1954296951040334464 20260525.3473 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 25.3473 2461185.8473 12.34 21:26:25.71 +40:35:04.0
86.27018 -7.26111 galactic Cyg Second-epoch detections are separated by 4.0" and 6.1 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 | 21:26:25.71 +40:35:04.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.408+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:25.71 +40:35:04.0: 12.64 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:25.71 +40:35:04.0: 14.68 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.58 +/- 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,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.00 21:16:04.57 +33:22:48.2
79.58762 -10.81406 galactic Cyg Second-epoch detections are separated by 3.8" and 7.7 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 | 21:16:04.57 +33:22:48.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:04.57 +33:22:48.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:04.57 +33:22:48.2: 14.33 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.33 +/- 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,2461185.8473,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:19:12.66 +42:09:19.6
86.42406 -5.19282 galactic Cyg Second-epoch detections are separated by 1.7" and 6.4 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 | Large-amplitude variable Gaia DR2 1968901660916555008 | 21:19:12.66 +42:09:19.6 (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=0.616+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:12.66 +42:09:19.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:12.66 +42:09:19.6: 14.84 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.84 +/- 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
Large-amplitude variable Gaia DR2 1968901660916555008,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1968901660916555008 20260525.3473 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 25.3473 2461185.8473 12.05 21:20:48.36 +38:04:38.6
83.70478 -8.26403 galactic Cyg Second-epoch detections are separated by 2.1" and 6.7 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 | 21:20:48.36 +38:04:38.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:48.36 +38:04:38.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:48.36 +38:04:38.6: 14.87 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.87 +/- 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,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.16 21:22:24.73 +38:01:28.6
83.89073 -8.52656 galactic Cyg Second-epoch detections are separated by 2.2" and 6.5 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 | 21:22:24.73 +38:01:28.6 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.042 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:24.73 +38:01:28.6: 13.01 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:24.73 +38:01:28.6: 14.77 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:13:13.48 +40:55:44.5
84.75677 -5.23451 galactic Cyg Second-epoch detections are separated by 2.2" and 7.0 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 | 21:13:13.48 +40:55:44.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:13.48 +40:55:44.5: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:13.48 +40:55:44.5: 14.63 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.63 +/- 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,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.14 21:33:16.02 +41:46:48.1
88.04059 -7.28669 galactic Cyg Second-epoch detections are separated by 2.7" and 7.1 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 J323.3240+41.7774 | 21:33:16.02 +41:46:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.474+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:16.02 +41:46:48.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:16.02 +41:46:48.1: 14.40 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.40 +/- 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+41.7774,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.20 21:16:51.47 +38:35:43.6
83.53742 -7.34735 galactic Cyg Second-epoch detections are separated by 1.9" and 6.4 pix
The object was found in VSX20" Gaia DR3 1964835151524796800
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.360 G 14.380 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:51.47 +38:35:43.6: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:51.47 +38:35:43.6: 14.48 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.48 +/- 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 1964835151524796800,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1964835151524796800 20260525.3473 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 25.3473 2461185.8473 12.28 21:49:04.94 +37:22:34.1
87.36405 -12.59913 galactic Cyg Second-epoch detections are separated by 1.9" and 7.3 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 | 21:49:04.94 +37:22:34.1 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:04.94 +37:22:34.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:04.94 +37:22:34.1: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.65 +/- 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,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.14 21:28:43.64 +35:42:00.9
83.13134 -11.06383 galactic Cyg Second-epoch detections are separated by 5.1" and 6.3 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 | 21:28:43.64 +35:42:00.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.64 +35:42:00.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.64 +35:42:00.9: 15.14 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.14 +/- 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,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.16 21:20:06.71 +36:34:21.2
82.51620 -9.21454 galactic Cyg Second-epoch detections are separated by 1.0" and 6.9 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 J320.0361+36.5707 | 21:20:06.71 +36:34:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:06.71 +36:34:21.2: 12.87 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:06.71 +36:34:21.2: 14.52 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 J320.0361+36.5707,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.0361+36.5707 20260525.3473 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 25.3473 2461185.8473 12.32 21:15:57.26 +39:30:06.5
84.07568 -6.59449 galactic Cyg Second-epoch detections are separated by 2.0" and 7.0 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 | 21:15:57.26 +39:30:06.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:57.26 +39:30:06.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:57.26 +39:30:06.5: 14.65 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.65 +/- 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,2461185.8473,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.18 21:31:29.67 +33:55:39.5
82.27747 -12.72714 galactic Cyg Second-epoch detections are separated by 4.4" and 6.8 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 | 21:31:29.67 +33:55:39.5 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:29.67 +33:55:39.5: 12.89 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:29.67 +33:55:39.5: 14.46 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.34 21:10:23.61 +41:02:56.4
84.47883 -4.76210 galactic Cyg Second-epoch detections are separated by 1.4" and 6.8 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 | 21:10:23.61 +41:02:56.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:23.61 +41:02:56.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:23.61 +41:02:56.4: 14.46 +/- 0.18 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
target,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:30:05.02 +40:57:00.0
87.02799 -7.47967 galactic Cyg Second-epoch detections are separated by 3.6" and 6.2 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 | 21:30:05.02 +40:57:00.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:05.02 +40:57:00.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:05.02 +40:57:00.0: 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.18 21:24:21.77 +38:05:16.5
84.20988 -8.75439 galactic Cyg Second-epoch detections are separated by 1.5" and 6.6 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 J321.0921+38.0906 | 21:24:21.77 +38:05:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:21.77 +38:05:16.5: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:21.77 +38:05:16.5: 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 J321.0921+38.0906,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.0921+38.0906 20260525.3473 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 25.3473 2461185.8473 12.18 21:22:55.49 +41:49:49.9
86.68022 -5.91166 galactic Cyg Second-epoch detections are separated by 1.4" and 6.4 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 J320.7324+41.8309 | 21:22:55.49 +41:49:49.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:22:55.49 +41:49:49.9: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:22:55.49 +41:49:49.9: 14.95 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.95 +/- 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 J320.7324+41.8309,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.7324+41.8309 20260525.3473 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 25.3473 2461185.8473 12.38 21:50:40.28 +40:44:27.7
89.82342 -10.23123 galactic Cyg Second-epoch detections are separated by 5.4" and 6.1 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 J327.6720+40.7392 | 21:50:40.28 +40:44:27.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:40.28 +40:44:27.7: 12.85 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:40.28 +40:44:27.7: 14.95 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 J327.6720+40.7392,2461185.8473,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J327.6720+40.7392 20260525.3473 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 25.3473 2461185.8473 12.27 21:16:10.43 +38:43:55.8
83.54418 -7.15637 galactic Cyg Second-epoch detections are separated by 2.5" and 7.1 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 | 21:16:10.43 +38:43:55.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:10.43 +38:43:55.8: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:10.43 +38:43:55.8: 14.85 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.85 +/- 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,2461185.8473,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.29 21:12:05.84 +40:41:57.5
84.44198 -5.23610 galactic Cyg Second-epoch detections are separated by 3.2" and 6.1 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 | 21:12:05.84 +40:41:57.5 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:05.84 +40:41:57.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:05.84 +40:41:57.5: 14.60 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.60 +/- 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,2461185.8473,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:30:39.37 +38:36:13.0
85.46747 -9.25003 galactic Cyg Second-epoch detections are separated by 0.8" and 7.0 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 J322.6569+38.5994 | 21:30:39.37 +38:36:13.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.349+/-0.046 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:39.37 +38:36:13.0: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:39.37 +38:36:13.0: 14.67 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.67 +/- 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+38.5994,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.12 21:16:40.15 +37:19:35.9
82.58485 -8.19616 galactic Cyg Second-epoch detections are separated by 4.7" and 6.5 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 J319.1753+37.3192 | 21:16:40.15 +37:19:35.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:40.15 +37:19:35.9: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:40.15 +37:19:35.9: 14.45 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.45 +/- 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 J319.1753+37.3192,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1753+37.3192 20260525.3473 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 25.3473 2461185.8473 12.11 21:19:47.74 +36:39:52.8
82.53858 -9.10490 galactic Cyg Second-epoch detections are separated by 4.7" and 6.5 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 J319.9416+36.6573 | 21:19:47.74 +36:39:52.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.658+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:47.74 +36:39:52.8: 12.66 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:47.74 +36:39:52.8: 14.50 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 J319.9416+36.6573,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.9416+36.6573 20260525.3473 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 25.3473 2461185.8473 12.11 21:19:40.11 +38:12:51.7
83.64618 -8.00827 galactic Cyg Second-epoch detections are separated by 1.0" and 7.0 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 | 21:19:40.11 +38:12:51.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:40.11 +38:12:51.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:40.11 +38:12:51.7: 14.81 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.81 +/- 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,2461185.8473,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.37 21:14:46.67 +40:23:26.2
84.56700 -5.81844 galactic Cyg Second-epoch detections are separated by 2.4" and 6.3 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 J318.6982+40.3853 | 21:14:46.67 +40:23:26.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.930+/-0.029 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:46.67 +40:23:26.2: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:46.67 +40:23:26.2: 14.46 +/- 0.18 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 J318.6982+40.3853,2461185.8473,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.6982+40.3853 20260525.3473 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 25.3473 2461185.8473 12.26 21:18:11.75 +41:23:26.2
85.74148 -5.59157 galactic Cyg Second-epoch detections are separated by 0.9" and 6.5 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 | 21:18:11.75 +41:23:26.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:11.75 +41:23:26.2: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:11.75 +41:23:26.2: 14.90 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.90 +/- 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,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.16 21:16:03.59 +37:34:29.4
82.68249 -7.93755 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 J319.0224+37.5558 | 21:16:05.55 +37:33:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.419+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:03.59 +37:34:29.4: 12.96 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:03.59 +37:34:29.4: 14.40 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 J319.0224+37.5558,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.0224+37.5558 20260525.3473 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 25.3473 2461185.8473 12.34 21:11:48.52 +42:10:15.8
85.48348 -4.19130 galactic Cyg Second-epoch detections are separated by 1.3" and 6.6 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 | 21:11:48.52 +42:10:15.8 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:48.52 +42:10:15.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:48.52 +42:10:15.8: 15.02 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.02 +/- 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,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.18 21:31:06.80 +39:46:47.2
86.35526 -8.46152 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 | 21:31:06.80 +39:46:47.2 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:06.80 +39:46:47.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:06.80 +39:46:47.2: 14.81 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.81 +/- 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,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.20 21:18:56.70 +40:10:47.9
84.96821 -6.53735 galactic Cyg Second-epoch detections are separated by 0.6" and 6.6 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 | 21:18:56.70 +40:10:47.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:56.70 +40:10:47.9: 12.41 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:56.70 +40:10:47.9: 14.43 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.36 +/- 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,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.07 21:28:06.54 +36:36:22.2
83.68750 -10.33061 galactic Cyg Second-epoch detections are separated by 4.0" and 6.2 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 J322.0278+36.6086 | 21:28:06.54 +36:36:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.343+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:06.54 +36:36:22.2: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:06.54 +36:36:22.2: 14.32 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.32 +/- 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 J322.0278+36.6086,2461185.8473,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.0278+36.6086 20260525.3473 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 25.3473 2461185.8473 12.28 21:15:24.90 +41:05:36.9
85.16222 -5.42115 galactic Cyg Second-epoch detections are separated by 0.6" and 6.5 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 J318.8500+41.1044 | 21:15:24.90 +41:05:36.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:24.90 +41:05:36.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:24.90 +41:05:36.9: 14.52 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.52 +/- 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 J318.8500+41.1044,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.8500+41.1044 20260525.3473 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 25.3473 2461185.8473 12.10 21:20:28.77 +35:50:51.5
82.04032 -9.77195 galactic Cyg Second-epoch detections are separated by 1.0" and 7.0 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 | 21:20:28.77 +35:50:51.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:28.77 +35:50:51.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:28.77 +35:50:51.5: 14.42 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.42 +/- 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,2461185.8473,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.49 21:11:22.27 +42:02:10.8
85.32923 -4.22399 galactic Cyg Second-epoch detections are separated by 3.3" and 6.5 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 | 21:11:22.27 +42:02:10.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:11:22.27 +42:02:10.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:11:22.27 +42:02:10.8: 14.77 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.77 +/- 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,2461185.8473,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:21:21.34 +38:00:17.5
83.72894 -8.39209 galactic Cyg Second-epoch detections are separated by 1.4" and 6.6 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 | 21:21:21.34 +38:00:17.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:21.34 +38:00:17.5: 13.26 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:21.34 +38:00:17.5: 14.32 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.27 21:24:31.55 +35:05:22.6
82.07464 -10.89096 galactic Cyg Second-epoch detections are separated by 0.7" and 7.0 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 | 21:24:31.55 +35:05:22.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:31.55 +35:05:22.6: 12.86 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:31.55 +35:05:22.6: 14.87 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461185.8473,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.20 21:15:06.19 +37:57:17.8
82.82995 -7.53895 galactic Cyg Second-epoch detections are separated by 0.9" and 6.8 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 J318.7737+37.9580 | 21:15:06.19 +37:57:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:06.19 +37:57:17.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:06.19 +37:57:17.8: 14.57 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.57 +/- 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 J318.7737+37.9580,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.7737+37.9580 20260525.3473 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 25.3473 2461185.8473 12.05 22:22:57.31 +41:08:15.2
95.05673 -13.56097 galactic Lac Second-epoch detections are separated by 2.7" and 7.5 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 | 22:22:57.31 +41:08:15.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:57.31 +41:08:15.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:57.31 +41:08:15.2: 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,2461185.8473,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.12 21:32:05.87 +40:41:03.1
87.12198 -7.93486 galactic Cyg Second-epoch detections are separated by 1.7" and 6.8 pix
The object was found in VSX 1" ASASSN-V J213205.93+404103.1
Type: SR
# Max. Min./Amp. JD0 Period
14.700 V 15.800 V 2457135.10000 99.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:05.87 +40:41:03.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:05.87 +40:41:03.1: 15.33 +/- 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
ASASSN-V J213205.93+404103.1,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213205.93+404103.1 20260525.3473 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 25.3473 2461185.8473 12.19 21:17:05.36 +42:12:57.9
86.19246 -4.86891 galactic Cyg Second-epoch detections are separated by 0.5" and 6.6 pix
The object was found in VSX 4" Gaia DR3 1969072875493929856
Type: RS
# Max. Min./Amp. JD0 Period
14.380 G 14.490 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:05.36 +42:12:57.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:05.36 +42:12:57.9: 14.60 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.60 +/- 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 1969072875493929856,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1969072875493929856 20260525.3473 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 25.3473 2461185.8473 12.43 21:33:08.65 +41:21:51.9
87.73737 -7.57454 galactic Cyg Second-epoch detections are separated by 0.3" and 6.8 pix
The object was found in VSX 2" Gaia DR3 1966368489204599552
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.530 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:08.65 +41:21:51.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:08.65 +41:21:51.9: 15.18 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.18 +/- 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
Gaia DR3 1966368489204599552,2461185.8473,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1966368489204599552 20260525.3473 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 25.3473 2461185.8473 12.19 21:12:36.49 +35:14:51.9
80.48424 -9.01935 galactic Cyg Second-epoch detections are separated by 2.7" and 6.6 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 | 21:12:36.49 +35:14:51.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:36.49 +35:14:51.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:36.49 +35:14:51.9: 14.54 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.54 +/- 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.19 21:46:24.52 +41:13:01.9
89.51311 -9.34779 galactic Cyg Second-epoch detections are separated by 2.5" and 6.6 pix
The object was found in ASASSN-V 4" ASASSN-V J214624.75+411304.6
Type: L
MeanMag 14.83 m Amp. 0.13 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:24.52 +41:13:01.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:24.52 +41:13:01.9: 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
VARIABLE_NAME,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.3473 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 25.3473 2461185.8473 12.34 21:28:44.93 +38:10:24.2
84.89221 -9.29947 galactic Cyg Second-epoch detections are separated by 1.7" and 6.9 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 J322.1854+38.1746 | 21:28:44.93 +38:10:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.064 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:44.93 +38:10:24.2: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:44.93 +38:10:24.2: 15.09 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.09 +/- 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
ATO J322.1854+38.1746,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.1854+38.1746 20260525.3473 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 25.3473 2461185.8473 12.18 21:18:22.26 +37:39:43.5
83.06550 -8.20822 galactic Cyg Second-epoch detections are separated by 0.5" and 6.9 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 | 21:18:22.26 +37:39:43.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:18:22.26 +37:39:43.5: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:18:22.26 +37:39:43.5: 14.49 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.49 +/- 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,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.12 21:19:08.62 +35:54:15.9
81.89133 -9.53769 galactic Cyg Second-epoch detections are separated by 2.3" and 6.9 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 J319.7934+35.9017 | 21:19:08.62 +35:54:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.430+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:08.62 +35:54:15.9: 13.00 +/- 0.27 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:08.62 +35:54:15.9: 14.47 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 J319.7934+35.9017,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.7934+35.9017 20260525.3473 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 25.3473 2461185.8473 12.34 21:23:44.88 +38:52:26.7
84.68620 -8.11366 galactic Cyg Second-epoch detections are separated by 4.0" and 6.1 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 J320.9332+38.8647 | 21:23:44.88 +38:52:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:44.88 +38:52:26.7: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:44.88 +38:52:26.7: 14.99 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.99 +/- 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 J320.9332+38.8647,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.9332+38.8647 20260525.3473 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 25.3473 2461185.8473 12.26 21:37:50.58 +36:54:52.2
85.34061 -11.45339 galactic Cyg Second-epoch detections are separated by 2.9" and 7.2 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 J324.4577+36.9154 | 21:37:50.58 +36:54:52.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:50.58 +36:54:52.2: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:50.58 +36:54:52.2: 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 J324.4577+36.9154,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.4577+36.9154 20260525.3473 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 25.3473 2461185.8473 12.17 21:38:19.56 +39:47:35.3
87.39059 -9.39639 galactic Cyg Second-epoch detections are separated by 2.0" and 6.6 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 J324.5932+39.7857 | 21:38:19.56 +39:47:35.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:19.56 +39:47:35.3: 13.27 +/- 0.30 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.56 +39:47:35.3: 14.89 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.34 +/- 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+39.7857,2461185.8473,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.18 22:21:26.07 +42:04:44.1
95.34903 -12.61975 galactic Lac Second-epoch detections are separated by 3.4" and 7.0 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 J335.3676+42.0840 | 22:21:26.07 +42:04:44.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:26.07 +42:04:44.1: 12.71 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:26.07 +42:04:44.1: 15.06 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 J335.3676+42.0840,2461185.8473,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.3676+42.0840 20260525.3473 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 25.3473 2461185.8473 12.26 21:50:17.58 +42:04:56.8
90.64064 -9.15628 galactic Cyg Second-epoch detections are separated by 2.4" and 6.5 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:17.58 +42:04:56.8: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:17.58 +42:04:56.8: 14.59 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.59 +/- 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 1960632160939763456,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.34 21:23:42.42 +39:12:33.7
84.92006 -7.87109 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 pix
The object was found in VSX 1" Gaia DR3 1965298045916380928
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.900 G 14.930 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:42.42 +39:12:33.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:42.42 +39:12:33.7: 14.72 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 1965298045916380928,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1965298045916380928 20260525.3473 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 25.3473 2461185.8473 12.15 21:24:07.47 +35:25:05.5
82.25407 -10.60182 galactic Cyg Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 6" Gaia DR3 1951537142496779264
Type: ROT
# Max. Min./Amp. JD0 Period
14.120 G 14.170 G 1.318000000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:07.47 +35:25:05.5: 12.71 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:07.47 +35:25:05.5: 14.34 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 1951537142496779264,2461185.8473,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1951537142496779264 20260525.3473 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 25.3473 2461185.8473 12.20 21:19:21.90 +41:32:54.8
86.00876 -5.63802 galactic Cyg Second-epoch detections are separated by 2.2" and 7.0 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 | 21:19:21.90 +41:32:54.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:19:21.90 +41:32:54.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:19:21.90 +41:32:54.8: 14.42 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.42 +/- 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,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:17:35.04 +42:45:34.5
86.64775 -4.55614 galactic Cyg Second-epoch detections are separated by 1.5" and 6.3 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 J319.3878+42.7571 | 21:17:35.04 +42:45:34.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:35.04 +42:45:34.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:35.04 +42:45:34.5: 14.88 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.88 +/- 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 J319.3878+42.7571,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.3878+42.7571 20260525.3473 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 25.3473 2461185.8473 12.28 21:34:40.18 +37:29:31.8
85.27139 -10.59995 galactic Cyg Second-epoch detections are separated by 1.8" and 7.1 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 1952180970973104128 | 21:34:42.69 +37:29:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.770+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:40.18 +37:29:31.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:40.18 +37:29:31.8: 14.57 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.57 +/- 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 1952180970973104128,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1952180970973104128 20260525.3473 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 25.3473 2461185.8473 12.14 21:28:43.59 +35:11:00.7
82.76139 -11.43172 galactic Cyg Second-epoch detections are separated by 2.7" and 7.4 pix
The object was found in VSX 5" 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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.59 +35:11:00.7: 12.89 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.59 +35:11:00.7: 14.42 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 1951299235669161728,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.21 21:43:18.74 +42:12:53.6
89.73225 -8.21539 galactic Cyg Second-epoch detections are separated by 2.6" and 6.4 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 | 21:43:18.74 +42:12:53.6 (user input) | T | P | (position from user input) J-Ks=1.126+/- (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:18.74 +42:12:53.6: 12.92 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:18.74 +42:12:53.6: 14.69 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.28 21:14:57.38 +39:59:29.7
84.29963 -6.11789 galactic Cyg Second-epoch detections are separated by 2.8" and 7.1 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 J318.7389+39.9897 | 21:14:57.38 +39:59:29.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:57.38 +39:59:29.7: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:57.38 +39:59:29.7: 14.80 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.80 +/- 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 J318.7389+39.9897,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.7389+39.9897 20260525.3473 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 25.3473 2461185.8473 12.16 21:32:16.35 +41:10:14.6
87.48315 -7.60360 galactic Cyg Second-epoch detections are separated by 2.1" and 6.6 pix
The object was found in VSX 9" ZTF J213215.55+411016.2
Type: EW
# Max. Min./Amp. JD0 Period
17.504 r Y 0.589 r 2458582.96660 0.318339600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:16.35 +41:10:14.6: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:16.35 +41:10:14.6: 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
ZTF J213215.55+411016.2,2461185.8473,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213215.55+411016.2 20260525.3473 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 25.3473 2461185.8473 12.20 21:13:17.09 +40:02:29.8
84.11523 -5.85088 galactic Cyg Second-epoch detections are separated by 0.6" and 6.7 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 J318.3329+40.0456 | 21:13:17.09 +40:02:29.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:17.09 +40:02:29.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:17.09 +40:02:29.8: 14.41 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.41 +/- 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 J318.3329+40.0456,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.3329+40.0456 20260525.3473 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 25.3473 2461185.8473 12.31 21:37:42.98 +40:11:43.1
87.57767 -9.02054 galactic Cyg Second-epoch detections are separated by 3.4" and 7.3 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 J324.4248+40.1975 | 21:37:42.98 +40:11:43.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:42.98 +40:11:43.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:42.98 +40:11:43.1: 14.75 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.75 +/- 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 J324.4248+40.1975,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.4248+40.1975 20260525.3473 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 25.3473 2461185.8473 12.32 21:30:38.52 +36:36:07.3
84.05450 -10.68871 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 | 21:30:38.52 +36:36:07.3 (user input) | T | P | (position from user input) J-Ks=0.605+/-0.060 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:38.52 +36:36:07.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:38.52 +36:36:07.3: 14.99 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.99 +/- 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,2461185.8473,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.21 21:12:32.95 +42:38:46.0
85.92455 -3.96591 galactic Cyg Second-epoch detections are separated by 3.0" and 7.0 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 J318.1347+42.6461 | 21:12:32.95 +42:38:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:32.95 +42:38:46.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:32.95 +42:38:46.0: 14.93 +/- 0.30 detection
Forced photometry reference-image weighted average: 14.93 +/- 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 J318.1347+42.6461,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.1347+42.6461 20260525.3473 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 25.3473 2461185.8473 12.32 21:37:44.49 +42:39:12.3
89.25124 -7.20463 galactic Cyg Second-epoch detections are separated by 3.9" and 6.1 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 | 21:37:44.49 +42:39:12.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:44.49 +42:39:12.3: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:44.49 +42:39:12.3: 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,2461185.8473,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.37 21:46:20.85 +36:51:37.6
86.59575 -12.63143 galactic Cyg Second-epoch detections are separated by 2.5" and 6.9 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 1952522025734029696 | 21:46:23.20 +36:51:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.588+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:20.85 +36:51:37.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:20.85 +36:51:37.6: 15.32 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.32 +/- 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 1952522025734029696,2461185.8473,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1952522025734029696 20260525.3473 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 25.3473 2461185.8473 12.45 21:44:15.84 +42:45:31.0
90.22643 -7.92041 galactic Cyg Second-epoch detections are separated by 4.7" and 7.5 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 | 21:44:15.84 +42:45:31.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:15.84 +42:45:31.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:15.84 +42:45:31.0: 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,2461185.8473,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:26:53.39 +40:39:04.3
86.38032 -7.27459 galactic Cyg Second-epoch detections are separated by 5.6" and 7.7 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 | 21:26:53.39 +40:39:04.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:53.39 +40:39:04.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:53.39 +40:39:04.3: 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.21 22:00:32.83 +39:39:03.1
90.61691 -12.26566 galactic Lac Second-epoch detections are separated by 1.7" and 7.1 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 1956210754106583168 | 22:00:31.09 +39:38:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:32.83 +39:39:03.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:32.83 +39:39:03.1: 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 1956210754106583168,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1956210754106583168 20260525.3473 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 25.3473 2461185.8473 12.14 21:20:55.89 +42:02:27.8
86.56717 -5.50046 galactic Cyg Second-epoch detections are separated by 3.5" and 7.1 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 J320.2347+42.0456 | 21:20:55.89 +42:02:27.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.529+/-0.077 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:55.89 +42:02:27.8: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:55.89 +42:02:27.8: 15.05 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.05 +/- 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 J320.2347+42.0456,2461185.8473,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.2347+42.0456 20260525.3473 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 25.3473 2461185.8473 12.36 21:54:33.42 +35:50:15.0
87.20372 -14.48328 galactic Peg Second-epoch detections are separated by 2.9" and 7.4 pix
The object was found in VSX 4" V0476 Peg
Type: UGSU
# Max. Min./Amp. JD0 Period
14.000 B 18.100 B 0.063700000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:33.42 +35:50:15.0: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:33.42 +35:50:15.0: 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
V0476 Peg,2461185.8473,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0476 Peg 20260525.3473 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 25.3473 2461185.8473 12.12 21:55:49.52 +34:16:12.7
86.36869 -15.85233 galactic Peg Second-epoch detections are separated by 0.5" and 7.3 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 | 21:55:49.52 +34:16:12.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:49.52 +34:16:12.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:49.52 +34:16:12.7: 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
target,2461185.8473,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.35 21:58:49.37 +40:28:42.2
90.87603 -11.41166 galactic Lac Second-epoch detections are separated by 0.6" and 7.1 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 | 21:58:49.37 +40:28:42.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:49.37 +40:28:42.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:49.37 +40:28:42.2: 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,2461185.8473,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.17 21:25:47.96 +38:44:14.8
84.87501 -8.49245 galactic Cyg Second-epoch detections are separated by 0.2" and 6.7 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 | 21:25:47.96 +38:44:14.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:47.96 +38:44:14.8: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:47.96 +38:44:14.8: 14.62 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.62 +/- 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,2461185.8473,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:23:15.52 +40:06:52.5
85.50436 -7.17014 galactic Cyg Second-epoch detections are separated by 1.5" and 7.0 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 | 21:23:15.52 +40:06:52.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:15.52 +40:06:52.5: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:15.52 +40:06:52.5: 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
target,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.43 21:21:11.28 +40:12:36.3
85.29174 -6.82216 galactic Cyg Second-epoch detections are separated by 1.4" and 6.8 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 | 21:21:11.28 +40:12:36.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:11.28 +40:12:36.3: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:11.28 +40:12:36.3: 14.83 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.83 +/- 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,2461185.8473,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.29 21:17:26.71 +36:06:08.9
81.79596 -9.15250 galactic Cyg Second-epoch detections are separated by 2.5" and 6.7 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 | 21:17:26.71 +36:06:08.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:17:26.71 +36:06:08.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:17:26.71 +36:06:08.9: 14.56 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.56 +/- 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,2461185.8473,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.24 22:11:18.63 +39:15:04.6
92.06931 -13.83878 galactic Lac Second-epoch detections are separated by 2.0" and 7.3 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 | 22:11:18.63 +39:15:04.6 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:11:18.63 +39:15:04.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:11:18.63 +39:15:04.6: 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,2461185.8473,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:38:11.91 +37:42:54.7
85.94691 -10.91270 galactic Cyg Second-epoch detections are separated by 0.8" and 7.0 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 J324.5379+37.7193 | 21:38:11.91 +37:42:54.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:11.91 +37:42:54.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:11.91 +37:42:54.7: 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
ATO J324.5379+37.7193,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.5379+37.7193 20260525.3473 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 25.3473 2461185.8473 12.30 21:38:48.53 +41:18:14.6
88.48652 -8.33866 galactic Cyg Second-epoch detections are separated by 1.2" and 6.6 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 | 21:38:48.53 +41:18:14.6 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:48.53 +41:18:14.6: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:48.53 +41:18:14.6: 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,2461185.8473,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.19 21:14:03.44 +35:50:46.0
81.13137 -8.82903 galactic Cyg Second-epoch detections are separated by 3.2" and 6.7 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 | 21:14:03.44 +35:50:46.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:03.44 +35:50:46.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:03.44 +35:50:46.0: 14.54 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.54 +/- 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.29 21:41:20.41 +36:37:18.6
85.66645 -12.14217 galactic Cyg Second-epoch detections are separated by 3.3" and 7.0 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 | 21:41:20.41 +36:37:18.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.861+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:20.41 +36:37:18.6: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:20.41 +36:37:18.6: 15.04 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.04 +/- 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,2461185.8473,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:21:30.19 +39:05:33.9
84.53278 -7.64995 galactic Cyg Second-epoch detections are separated by 0.3" and 6.8 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 | 21:21:30.19 +39:05:33.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:30.19 +39:05:33.9: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:30.19 +39:05:33.9: 14.43 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.21 21:37:02.07 +39:22:40.0
86.92020 -9.53481 galactic Cyg Second-epoch detections are separated by 1.7" and 6.9 pix
The object was found in VSX 9" Gaia DR3 1953948096617832576
Type: ROT
# Max. Min./Amp. JD0 Period
17.180 G 17.250 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:02.07 +39:22:40.0: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:02.07 +39:22:40.0: 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
Gaia DR3 1953948096617832576,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1953948096617832576 20260525.3473 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 25.3473 2461185.8473 12.31 21:29:02.36 +41:37:46.7
87.35913 -6.85322 galactic Cyg Second-epoch detections are separated by 0.6" and 6.7 pix
The object was found in VSX 3" ZTF J212902.50+413749.5
Type: RS
# Max. Min./Amp. JD0 Period
14.642 r Y 0.039 r 2458363.76860 0.352450800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:02.36 +41:37:46.7: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:02.36 +41:37:46.7: 15.01 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.01 +/- 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
ZTF J212902.50+413749.5,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212902.50+413749.5 20260525.3473 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 25.3473 2461185.8473 12.52 21:31:05.87 +41:04:08.3
87.25048 -7.52551 galactic Cyg Second-epoch detections are separated by 1.1" and 6.6 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 | 21:31:05.87 +41:04:08.3 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.055 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:05.87 +41:04:08.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:05.87 +41:04:08.3: 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
target,2461185.8473,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.35 21:10:16.74 +40:21:12.6
83.95142 -5.21832 galactic Cyg Second-epoch detections are separated by 1.8" and 6.8 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 J317.5588+40.3458 | 21:10:16.74 +40:21:12.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:10:16.74 +40:21:12.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:10:16.74 +40:21:12.6: 14.59 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.59 +/- 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 J317.5588+40.3458,2461185.8473,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J317.5588+40.3458 20260525.3473 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 25.3473 2461185.8473 12.23 21:53:37.45 +42:42:28.2
91.52413 -9.06473 galactic Cyg Second-epoch detections are separated by 2.0" and 6.8 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 | 21:53:37.45 +42:42:28.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:37.45 +42:42:28.2: 13.08 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:37.45 +42:42:28.2: 14.59 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:40:19.37 +35:38:56.5
84.84001 -12.72285 galactic Cyg Second-epoch detections are separated by 3.3" and 6.8 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 | 21:40:19.37 +35:38:56.5 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:19.37 +35:38:56.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:19.37 +35:38:56.5: 14.73 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.73 +/- 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,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.19 21:52:16.26 +42:41:08.0
91.31496 -8.92461 galactic Cyg Second-epoch detections are separated by 1.6" and 7.0 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 | 21:52:16.26 +42:41:08.0 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:16.26 +42:41:08.0: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:16.26 +42:41:08.0: 14.43 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.19 21:24:46.53 +35:05:09.9
82.10865 -10.92977 galactic Cyg Second-epoch detections are separated by 4.0" and 6.5 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 | 21:24:46.53 +35:05:09.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:46.53 +35:05:09.9: 12.56 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:46.53 +35:05:09.9: 14.98 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.27 21:21:59.18 +39:53:48.7
85.17560 -7.15104 galactic Cyg Second-epoch detections are separated by 3.5" and 6.5 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 | 21:21:59.18 +39:53:48.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:59.18 +39:53:48.7: 12.68 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:59.18 +39:53:48.7: 14.87 +/- 0.27 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,2461185.8473,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:15:04.85 +39:19:08.4
83.82529 -6.59821 galactic Cyg Second-epoch detections are separated by 1.9" and 6.7 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 | 21:15:04.85 +39:19:08.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:15:04.85 +39:19:08.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:15:04.85 +39:19:08.4: 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,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.21 21:13:00.22 +38:06:52.6
82.66206 -7.12825 galactic Cyg Second-epoch detections are separated by 3.3" and 6.5 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 J318.2534+38.1054 | 21:13:00.22 +38:06:52.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.294+/-0.036 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:00.22 +38:06:52.6: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:00.22 +38:06:52.6: 14.44 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 J318.2534+38.1054,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.2534+38.1054 20260525.3473 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 25.3473 2461185.8473 12.19 21:21:52.77 +34:43:08.5
81.41860 -10.76248 galactic Cyg Second-epoch detections are separated by 1.0" and 6.9 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 | 21:21:52.77 +34:43:08.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:52.77 +34:43:08.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:52.77 +34:43:08.5: 14.61 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.61 +/- 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,2461185.8473,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.25 21:41:27.40 +42:51:23.9
89.90047 -7.50763 galactic Cyg Second-epoch detections are separated by 1.0" and 6.6 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 | 21:41:27.40 +42:51:23.9 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.505+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:27.40 +42:51:23.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:27.40 +42:51:23.9: 14.40 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.40 +/- 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,2461185.8473,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 22:00:11.18 +39:37:38.7
90.54621 -12.24113 galactic Lac Second-epoch detections are separated by 2.0" and 7.3 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 | 22:00:11.18 +39:37:38.7 (user input) | T | P | (position from user input) J-Ks=1.010+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:11.18 +39:37:38.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:11.18 +39:37:38.7: 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
target,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.43 21:36:26.19 +42:23:45.7
88.89738 -7.23329 galactic Cyg Second-epoch detections are separated by 2.3" and 7.0 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 | 21:36:26.19 +42:23:45.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:26.19 +42:23:45.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:26.19 +42:23:45.7: 14.71 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.71 +/- 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,2461185.8473,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.30 21:09:49.64 +38:21:37.4
82.41739 -6.50342 galactic Cyg Second-epoch detections are separated by 1.6" and 7.0 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 | 21:09:49.64 +38:21:37.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:09:49.64 +38:21:37.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:09:49.64 +38:21:37.4: 14.27 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461185.8473,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.23 21:14:30.73 +35:31:36.4
80.95860 -9.11430 galactic Cyg Second-epoch detections are separated by 2.8" and 6.8 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 J318.6385+35.5209 | 21:14:30.73 +35:31:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.411+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:30.73 +35:31:36.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:30.73 +35:31:36.4: 14.44 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.44 +/- 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 J318.6385+35.5209,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.6385+35.5209 20260525.3473 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 25.3473 2461185.8473 12.36 21:46:05.72 +42:50:03.3
90.53332 -8.08234 galactic Cyg Second-epoch detections are separated by 2.6" and 7.2 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 | 21:46:05.72 +42:50:03.3 (user input) | T | P | (position from user input) J-Ks=0.720+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:05.72 +42:50:03.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:05.72 +42:50:03.3: 14.78 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.78 +/- 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,2461185.8473,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.35 21:28:40.79 +39:00:17.9
85.46934 -8.69385 galactic Cyg Second-epoch detections are separated by 1.9" and 7.0 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 J322.1768+39.0006 | 21:28:40.79 +39:00:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:40.79 +39:00:17.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:40.79 +39:00:17.9: 14.73 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.73 +/- 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 J322.1768+39.0006,2461185.8473,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.1768+39.0006 20260525.3473 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 25.3473 2461185.8473 12.46 21:45:01.25 +42:15:60.0
90.00781 -8.38368 galactic Cyg Second-epoch detections are separated by 0.8" and 7.0 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 | 21:45:01.25 +42:15:60.0 (user input) | T | P | (position from user input) J-Ks=0.858+/-0.027 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:01.25 +42:15:60.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:01.25 +42:15:60.0: 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,2461185.8473,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.40 21:33:09.21 +37:05:56.5
84.77359 -10.67822 galactic Cyg Second-epoch detections are separated by 1.0" and 7.0 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 | 21:33:09.21 +37:05:56.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:09.21 +37:05:56.5: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:09.21 +37:05:56.5: 15.00 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.00 +/- 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,2461185.8473,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.36 21:23:39.40 +38:42:01.8
84.54937 -8.22367 galactic Cyg Second-epoch detections are separated by 2.4" and 7.0 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 J320.9226+38.6956 | 21:23:39.40 +38:42:01.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:23:39.40 +38:42:01.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:23:39.40 +38:42:01.8: 14.73 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.73 +/- 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 J320.9226+38.6956,2461185.8473,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.9226+38.6956 20260525.3473 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 25.3473 2461185.8473 12.23 21:35:31.04 +33:55:25.7
82.89105 -13.30939 galactic Cyg Second-epoch detections are separated by 3.8" and 7.2 pix
The object was found in VSX 3" Gaia DR3 1950223427957054848
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.510 G 12.727600000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:31.04 +33:55:25.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:31.04 +33:55:25.7: 14.87 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.87 +/- 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 1950223427957054848,2461185.8473,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1950223427957054848 20260525.3473 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 25.3473 2461185.8473 12.30 21:28:13.70 +33:56:53.8
81.79837 -12.23669 galactic Cyg Second-epoch detections are separated by 3.1" and 7.3 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 | 21:28:13.70 +33:56:53.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:13.70 +33:56:53.8: 13.25 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:13.70 +33:56:53.8: 14.78 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461185.8473,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.49 21:32:31.54 +41:50:58.7
87.98692 -7.14146 galactic Cyg Second-epoch detections are separated by 0.4" and 6.7 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 J323.1140+41.8499 | 21:32:31.54 +41:50:58.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:31.54 +41:50:58.7: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:31.54 +41:50:58.7: 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 J323.1140+41.8499,2461185.8473,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.1140+41.8499 20260525.3473 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 25.3473 2461185.8473 12.36 21:32:41.02 +38:29:40.1
85.68174 -9.60270 galactic Cyg Second-epoch detections are separated by 0.7" and 6.9 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 | 21:32:41.02 +38:29:40.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:41.02 +38:29:40.1: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:41.02 +38:29:40.1: 14.49 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.49 +/- 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,2461185.8473,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:39:50.83 +41:51:15.2
89.00401 -8.05931 galactic Cyg Second-epoch detections are separated by 1.8" and 6.8 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 | 21:39:50.83 +41:51:15.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:50.83 +41:51:15.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:50.83 +41:51:15.2: 15.01 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.01 +/- 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.38 22:02:09.38 +41:51:02.7
92.24047 -10.71609 galactic Lac Second-epoch detections are separated by 3.1" and 7.4 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 | 22:02:09.38 +41:51:02.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:09.38 +41:51:02.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:09.38 +41:51:02.7: 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
target,2461185.8473,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.40 21:55:25.46 +41:56:48.8
91.30074 -9.86547 galactic Cyg Second-epoch detections are separated by 1.3" and 6.7 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 | 21:55:25.46 +41:56:48.8 (user input) | T | P | (position from user input) J-Ks=0.619+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:25.46 +41:56:48.8: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:25.46 +41:56:48.8: 14.57 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.57 +/- 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,2461185.8473,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.24 21:54:17.19 +36:52:11.4
87.84203 -13.65543 galactic Cyg Second-epoch detections are separated by 2.4" and 6.9 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 1949793420131211520 | 21:54:15.63 +36:52:54.0 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:17.19 +36:52:11.4: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:17.19 +36:52:11.4: 14.65 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 1949793420131211520,2461185.8473,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1949793420131211520 20260525.3473 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 25.3473 2461185.8473 12.41 21:26:28.37 +37:36:33.1
84.16691 -9.38753 galactic Cyg Second-epoch detections are separated by 2.0" and 7.2 pix
The object was found in VSX17" ZTF J212628.00+373617.0
Type: EW
# Max. Min./Amp. JD0 Period
16.581 r Y 0.338 r 2458382.81300 0.401864000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:28.37 +37:36:33.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:28.37 +37:36:33.1: 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
ZTF J212628.00+373617.0,2461185.8473,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J212628.00+373617.0 20260525.3473 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 25.3473 2461185.8473 12.39 21:21:23.84 +33:48:25.1
80.67998 -11.32482 galactic Cyg Second-epoch detections are separated by 2.9" and 7.6 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 | 21:21:23.84 +33:48:25.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:23.84 +33:48:25.1: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:23.84 +33:48:25.1: 14.84 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.84 +/- 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,2461185.8473,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.45 21:31:17.20 +37:57:30.7
85.10503 -9.80110 galactic Cyg Second-epoch detections are separated by 1.6" and 6.9 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 J322.8242+37.9583 | 21:31:17.20 +37:57:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.470+/-0.055 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:17.20 +37:57:30.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:17.20 +37:57:30.7: 14.81 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.81 +/- 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 J322.8242+37.9583,2461185.8473,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.21 21:14:45.84 +36:18:04.1
81.56642 -8.62279 galactic Cyg Second-epoch detections are separated by 1.6" and 7.0 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 1867815581211192064 | 21:14:45.84 +36:18:04.1 (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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:14:45.84 +36:18:04.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:14:45.84 +36:18:04.1: 14.80 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.80 +/- 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 1867815581211192064,2461185.8473,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1867815581211192064 20260525.3473 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 25.3473 2461185.8473 12.38 21:24:27.69 +40:15:21.0
85.76887 -7.23225 galactic Cyg Second-epoch detections are separated by 1.5" and 6.8 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 J321.1133+40.2583 | 21:24:27.69 +40:15:21.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:27.69 +40:15:21.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:27.69 +40:15:21.0: 15.26 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.26 +/- 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 J321.1133+40.2583,2461185.8473,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.1133+40.2583 20260525.3473 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 25.3473 2461185.8473 12.28 22:01:06.44 +42:14:35.8
92.32757 -10.28635 galactic Lac Second-epoch detections are separated by 1.7" and 7.0 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 | 22:01:06.44 +42:14:35.8 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:06.44 +42:14:35.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:06.44 +42:14:35.8: 15.10 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.10 +/- 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,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.40 21:16:12.44 +38:09:29.8
83.12964 -7.55683 galactic Cyg Second-epoch detections are separated by 2.4" and 6.4 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 J319.0671+38.1620 | 21:16:12.44 +38:09:29.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.706+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:16:12.44 +38:09:29.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:16:12.44 +38:09:29.8: 14.36 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 J319.0671+38.1620,2461185.8473,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.0671+38.1620 20260525.3473 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 25.3473 2461185.8473 12.26 21:28:18.00 +34:05:00.0
81.90663 -12.15146 galactic Cyg Second-epoch detections are separated by 3.4" and 7.5 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 | 21:28:18.00 +34:05:00.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:18.00 +34:05:00.0: 12.65 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:18.00 +34:05:00.0: 14.45 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.40 21:56:20.29 +42:31:29.4
91.80156 -9.52062 galactic Cyg Second-epoch detections are separated by 2.6" and 7.2 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 J329.0969+42.5237 | 21:56:20.29 +42:31:29.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.752+/-0.046 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:20.29 +42:31:29.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:20.29 +42:31:29.4: 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
ATO J329.0969+42.5237,2461185.8473,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J329.0969+42.5237 20260525.3473 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 25.3473 2461185.8473 12.43 21:35:50.10 +39:03:54.1
86.53193 -9.60689 galactic Cyg Second-epoch detections are separated by 1.1" and 6.8 pix
The object was found in VSX19" Gaia DR3 1953844605086798592
Type: ROT
# Max. Min./Amp. JD0 Period
16.260 G 16.280 G 0.468671000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:50.10 +39:03:54.1: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:50.10 +39:03:54.1: 15.14 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.14 +/- 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 1953844605086798592,2461185.8473,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1953844605086798592 20260525.3473 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 25.3473 2461185.8473 12.51 21:33:40.41 +40:44:24.3
87.38036 -8.09862 galactic Cyg Second-epoch detections are separated by 3.0" and 6.3 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 | 21:33:40.41 +40:44:24.3 (user input) | T | P | (position from user input) J-Ks=0.795+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:40.41 +40:44:24.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:40.41 +40:44:24.3: 14.86 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.86 +/- 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,2461185.8473,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.22 21:36:23.84 +37:34:30.9
85.58366 -10.77332 galactic Cyg Second-epoch detections are separated by 1.8" and 7.1 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 | 21:36:23.84 +37:34:30.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:23.84 +37:34:30.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:23.84 +37:34:30.9: 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
target,2461185.8473,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:20:02.87 +34:35:15.8
81.05629 -10.58257 galactic Cyg Second-epoch detections are separated by 1.0" and 6.9 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 | 21:20:02.87 +34:35:15.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:20:02.87 +34:35:15.8: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:20:02.87 +34:35:15.8: 14.93 +/- 0.31 detection
Forced photometry reference-image weighted average: 14.93 +/- 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,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.47 21:46:41.17 +40:55:18.6
89.35825 -9.60594 galactic Cyg Second-epoch detections are separated by 1.8" and 6.6 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 | 21:46:41.17 +40:55:18.6 (user input) | T | P | (position from user input) J-Ks=0.603+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:41.17 +40:55:18.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:41.17 +40:55:18.6: 14.98 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.98 +/- 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,2461185.8473,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.26 21:30:24.45 +39:13:33.0
85.86846 -8.76769 galactic Cyg Second-epoch detections are separated by 3.2" and 7.0 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 J322.6021+39.2250 | 21:30:24.45 +39:13:33.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:24.45 +39:13:33.0: 12.96 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:24.45 +39:13:33.0: 14.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 J322.6021+39.2250,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.6021+39.2250 20260525.3473 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 25.3473 2461185.8473 12.20 21:25:22.48 +36:07:15.0
82.94291 -10.28701 galactic Cyg Second-epoch detections are separated by 0.7" and 7.0 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 | 21:25:22.48 +36:07:15.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:22.48 +36:07:15.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:22.48 +36:07:15.0: 14.71 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.71 +/- 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,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.46 21:49:31.96 +39:23:33.6
88.77001 -11.12228 galactic Cyg Second-epoch detections are separated by 2.5" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1953379477305077120
Type: ROT
# Max. Min./Amp. JD0 Period
14.210 G 14.240 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:31.96 +39:23:33.6: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:31.96 +39:23:33.6: 15.01 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.01 +/- 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 1953379477305077120,2461185.8473,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1953379477305077120 20260525.3473 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 25.3473 2461185.8473 12.35 21:54:45.67 +38:18:18.0
88.85589 -12.60962 galactic Cyg Second-epoch detections are separated by 1.8" and 7.2 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 | 21:54:45.67 +38:18:18.0 (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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:45.67 +38:18:18.0: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:45.67 +38:18:18.0: 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,2461185.8473,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.31 21:24:23.57 +37:19:36.4
83.66860 -9.29624 galactic Cyg Second-epoch detections are separated by 1.1" and 6.9 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 | 21:24:23.57 +37:19:36.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:24:23.57 +37:19:36.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:24:23.57 +37:19:36.4: 14.84 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.84 +/- 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,2461185.8473,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.24 21:21:25.14 +36:00:11.8
82.28807 -9.80006 galactic Cyg Second-epoch detections are separated by 2.0" and 6.6 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 | 21:21:25.14 +36:00:11.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:21:25.14 +36:00:11.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:21:25.14 +36:00:11.8: 14.46 +/- 0.18 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
target,2461185.8473,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.20 22:09:31.96 +42:04:29.4
93.49539 -11.35897 galactic Lac Second-epoch detections are separated by 0.9" and 7.2 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 | 22:09:31.96 +42:04:29.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:31.96 +42:04:29.4: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:31.96 +42:04:29.4: 15.11 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.11 +/- 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,2461185.8473,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.28 21:25:13.85 +34:03:17.5
81.42762 -11.72116 galactic Cyg Second-epoch detections are separated by 1.6" and 6.8 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 | 21:25:13.85 +34:03:17.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:25:13.85 +34:03:17.5: 12.96 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:25:13.85 +34:03:17.5: 14.42 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461185.8473,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.40 21:32:24.91 +37:04:42.8
84.65081 -10.59140 galactic Cyg Second-epoch detections are separated by 1.9" and 6.6 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 | 21:32:24.91 +37:04:42.8 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.046 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:24.91 +37:04:42.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:24.91 +37:04:42.8: 15.36 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.36 +/- 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,2461185.8473,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 12.34 21:38:56.76 +37:31:12.5
85.92365 -11.15649 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 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 J324.7367+37.5110 | 21:38:56.76 +37:31:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:56.76 +37:31:12.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:56.76 +37:31:12.5: 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
ATO J324.7367+37.5110,2461185.8473,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.7367+37.5110 20260525.3473 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 25.3473 2461185.8473 12.26 21:40:15.33 +37:50:20.7
86.33778 -11.09531 galactic Cyg Second-epoch detections are separated by 0.8" and 6.8 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 | 21:40:15.33 +37:50:20.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.793+/-0.051 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:15.33 +37:50:20.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:15.33 +37:50:20.7: 13.83 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 J325.0657+37.8384,2461185.8473,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260525.3473 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 25.3473 2461185.8473 12.37 21:39:30.73 +37:21:41.9
85.89914 -11.34930 galactic Cyg Second-epoch detections are separated by 2.9" and 6.6 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 | 21:39:30.73 +37:21:41.9 (user input) | T | P | (position from user input) J-Ks=0.871+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:30.73 +37:21:41.9: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:30.73 +37:21:41.9: 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,2461185.8473,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 10.30 21:52:59.99 +33:25:12.1
85.33151 -16.12219 galactic Peg Second-epoch detections are separated by 1.2" and 7.4 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 J328.2515+33.4325 | 21:52:59.99 +33:25:12.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:59.99 +33:25:12.1: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:59.99 +33:25:12.1: 12.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 J328.2515+33.4325,2461185.8473,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J328.2515+33.4325 20260525.3473 10.30CV 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 25.3473 2461185.8473 10.10 22:25:38.96 +39:59:37.6
94.84913 -14.79769 galactic Lac Second-epoch detections are separated by 1.4" and 7.4 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 J336.4111+39.9905 | 22:25:39.07 +39:59:38.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.677+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:38.96 +39:59:37.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:38.96 +39:59:37.6: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 J336.4111+39.9905,2461185.8473,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.4111+39.9905 20260525.3473 10.10CV 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 25.3473 2461185.8473 9.56 22:23:25.16 +41:54:05.1
95.56372 -12.97145 galactic Lac Second-epoch detections are separated by 0.3" and 7.3 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 J335.8552+41.9019 | 22:23:25.26 +41:54:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.795+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:25.16 +41:54:05.1: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:25.16 +41:54:05.1: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.37 +/- 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 J335.8552+41.9019,2461185.8473,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.8552+41.9019 20260525.3473 9.56CV 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 25.3473 2461185.8473 10.29 22:17:10.57 +41:19:17.1
94.23864 -12.79944 galactic Lac Second-epoch detections are separated by 0.2" and 7.2 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 | 22:17:10.57 +41:19:17.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:17:10.57 +41:19:17.1: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:17:10.57 +41:19:17.1: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 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,2461185.8473,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.29CV 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 25.3473 2461185.8473 11.13 21:57:38.14 +32:57:13.0
85.79037 -17.10450 galactic Peg Second-epoch detections are separated by 1.8" and 7.1 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 | 21:57:38.14 +32:57:13.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:38.14 +32:57:13.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:38.14 +32:57:13.0: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461185.8473,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 11.47 22:18:25.69 +41:03:50.0
94.28772 -13.14514 galactic Lac Second-epoch detections are separated by 3.7" and 7.8 pix
The object was found in VSX22" Gaia DR3 1957319474142739712
Type: ROT
# Max. Min./Amp. JD0 Period
14.590 G 14.610 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:25.69 +41:03:50.0: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:25.69 +41:03:50.0: 14.07 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 1957319474142739712,2461185.8473,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957319474142739712 20260525.3473 11.47CV 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 25.3473 2461185.8473 8.56 22:23:57.60 +41:47:31.3
95.58846 -13.11816 galactic Lac Second-epoch detections are separated by 1.0" and 7.4 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 1957705883761638144 | 22:23:57.51 +41:47:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=-0.010+/-0.026 (A)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:57.60 +41:47:31.3: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:57.60 +41:47:31.3: 11.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 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 1957705883761638144,2461185.8473,8.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957705883761638144 20260525.3473 8.56CV 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 25.3473 2461185.8473 9.76 21:12:38.95 +33:09:36.0
78.92890 -10.43671 galactic Cyg Second-epoch detections are separated by 1.0" and 7.1 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 1866777234222282496 | 21:12:39.04 +33:09:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.679+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:12:38.95 +33:09:36.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:12:38.95 +33:09:36.0: 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
Gaia DR3 1866777234222282496,2461185.8473,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1866777234222282496 20260525.3473 9.76CV 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 25.3473 2461185.8473 10.87 22:24:39.80 +40:04:40.5
94.73363 -14.62386 galactic Lac Second-epoch detections are separated by 0.5" and 7.4 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 J336.1524+40.0725 | 22:24:39.80 +40:04:40.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:39.80 +40:04:40.5: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:39.80 +40:04:40.5: 13.83 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 J336.1524+40.0725,2461185.8473,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.1524+40.0725 20260525.3473 10.87CV 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 25.3473 2461185.8473 10.65 21:13:52.12 +34:18:26.4
79.96153 -9.84730 galactic Cyg Second-epoch detections are separated by 2.3" and 6.7 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 J318.4777+34.3152 | 21:13:52.12 +34:18:26.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:13:52.12 +34:18:26.4: 12.97 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:13:52.12 +34:18:26.4: 13.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 J318.4777+34.3152,2461185.8473,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.4777+34.3152 20260525.3473 10.65CV 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 25.3473 2461185.8473 11.59 22:27:04.57 +38:45:58.5
94.39344 -15.97660 galactic Lac Second-epoch detections are separated by 2.3" and 7.6 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 | 22:27:04.57 +38:45:58.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:04.57 +38:45:58.5: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:04.57 +38:45:58.5: 14.80 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.80 +/- 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,2461185.8473,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 11.59CV 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 25.3473 2461185.8473 11.77 21:50:32.90 +33:17:12.9
84.83797 -15.88825 galactic Peg Second-epoch detections are separated by 1.4" and 7.3 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 | 21:50:32.90 +33:17:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:32.90 +33:17:12.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:32.90 +33:17:12.9: 14.34 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461185.8473,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 9.61 21:28:06.78 +39:56:16.0
86.04677 -7.94843 galactic Cyg Second-epoch detections are separated by 0.8" and 6.8 pix
The object was found in VSX 2" V0837 Cyg
Type: M
# Max. Min./Amp. JD0 Period
13.800 B 17.100 B 2443192.00000 292.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:06.78 +39:56:16.0: 12.99 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:06.78 +39:56:16.0: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 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
V0837 Cyg,2461185.8473,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0837 Cyg 20260525.3473 9.61CV 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 25.3473 2461185.8473 10.72 22:24:05.20 +39:13:30.0
94.15104 -15.27422 galactic Lac Second-epoch detections are separated by 1.2" and 7.6 pix
The object was found in VSX14" Gaia DR3 1908853585705819648
Type: ROT
# Max. Min./Amp. JD0 Period
13.910 G 13.950 G 4.425460000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:05.20 +39:13:30.0: 12.74 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:05.20 +39:13:30.0: 13.64 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 1908853585705819648,2461185.8473,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1908853585705819648 20260525.3473 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 25.3473 2461185.8473 10.86 22:20:30.72 +33:13:11.8
89.96322 -19.81809 galactic Peg Second-epoch detections are separated by 1.2" and 7.7 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 | 22:20:30.72 +33:13:11.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:20:30.72 +33:13:11.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:20:30.72 +33:13:11.8: 14.04 +/- 0.12 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
target,2461185.8473,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.86CV 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 25.3473 2461185.8473 8.54 22:26:47.99 +39:55:16.8
94.99950 -14.97863 galactic Lac Second-epoch detections are separated by 0.6" and 7.4 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 1909266727200326784 | 22:26:48.06 +39:55:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.535+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:47.99 +39:55:16.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:47.99 +39:55:16.8: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 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 1909266727200326784,2461185.8473,8.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1909266727200326784 20260525.3473 8.54CV 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 25.3473 2461185.8473 8.59 22:27:15.22 +40:20:02.7
95.30651 -14.67895 galactic Lac Second-epoch detections are separated by 0.5" and 7.4 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 1909351252156975488 | 22:27:15.29 +40:20:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.654+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:15.22 +40:20:02.7: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:15.22 +40:20:02.7: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 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 1909351252156975488,2461185.8473,8.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1909351252156975488 20260525.3473 8.59CV 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 25.3473 2461185.8473 8.84 22:28:37.12 +40:06:52.2
95.41088 -15.00441 galactic Lac Second-epoch detections are separated by 0.5" and 7.4 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 1909287068167102592 | 22:28:37.24 +40:06:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.659+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:37.12 +40:06:52.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:37.12 +40:06:52.2: 11.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.87 +/- 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 1909287068167102592,2461185.8473,8.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1909287068167102592 20260525.3473 8.84CV 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 25.3473 2461185.8473 11.13 22:27:39.56 +42:05:42.1
96.35078 -13.23682 galactic Lac Second-epoch detections are separated by 1.5" and 7.6 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 | 22:27:39.56 +42:05:42.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:39.56 +42:05:42.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:39.56 +42:05:42.1: 13.96 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461185.8473,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 9.75 22:27:39.15 +41:18:21.0
95.91334 -13.90166 galactic Lac Second-epoch detections are separated by 0.8" and 7.4 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 J336.9135+41.3062 | 22:27:39.24 +41:18:22.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:39.15 +41:18:21.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:39.15 +41:18:21.0: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 J336.9135+41.3062,2461185.8473,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.9135+41.3062 20260525.3473 9.75CV 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 25.3473 2461185.8473 9.60 22:22:07.59 +40:53:07.5
94.77910 -13.68429 galactic Lac Second-epoch detections are separated by 0.5" and 7.3 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 1957466087146190336 | 22:22:07.67 +40:53:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.704+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:07.59 +40:53:07.5: 12.53 +/- 0.15 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:07.59 +40:53:07.5: 12.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 1957466087146190336,2461185.8473,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957466087146190336 20260525.3473 9.60CV 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 25.3473 2461185.8473 9.52 22:23:44.27 +32:54:14.5
90.35888 -20.46511 galactic Peg Second-epoch detections are separated by 0.2" and 7.6 pix
The object was found in VSX 1" ZTF J222344.31+325415.0
Type: SR
# Max. Min./Amp. JD0 Period
12.655 g Y 0.093 g 2458656.47660 63.170119700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:44.27 +32:54:14.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:44.27 +32:54:14.5: 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
ZTF J222344.31+325415.0,2461185.8473,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J222344.31+325415.0 20260525.3473 9.52CV 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 25.3473 2461185.8473 9.87 22:12:21.99 +33:37:10.3
88.75946 -18.49313 galactic Peg Second-epoch detections are separated by 0.2" and 7.4 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 1899339889547890816 | 22:12:22.04 +33:37:11.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.385+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:21.99 +33:37:10.3: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:21.99 +33:37:10.3: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 1899339889547890816,2461185.8473,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1899339889547890816 20260525.3473 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 25.3473 2461185.8473 9.84 22:24:47.11 +40:38:54.7
95.07698 -14.15960 galactic Lac Second-epoch detections are separated by 0.4" and 7.3 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 1957391870111667200 | 22:24:47.23 +40:38:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.706+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:47.11 +40:38:54.7: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:47.11 +40:38:54.7: 12.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 1957391870111667200,2461185.8473,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957391870111667200 20260525.3473 9.84CV 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 25.3473 2461185.8473 9.90 22:21:42.03 +36:19:16.6
92.04925 -17.41589 galactic Lac Second-epoch detections are separated by 0.3" and 7.5 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 1906006469065113728 | 22:21:42.10 +36:19:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:42.03 +36:19:16.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:42.03 +36:19:16.6: 12.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 1906006469065113728,2461185.8473,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1906006469065113728 20260525.3473 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 25.3473 2461185.8473 9.79 22:25:36.46 +40:51:52.1
95.33318 -14.06392 galactic Lac Second-epoch detections are separated by 0.3" and 7.4 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 1957417639915825536 | 22:25:36.48 +40:51:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.561+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:36.46 +40:51:52.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:36.46 +40:51:52.1: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 1957417639915825536,2461185.8473,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957417639915825536 20260525.3473 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 25.3473 2461185.8473 9.89 22:25:10.79 +41:11:46.2
95.44992 -13.74191 galactic Lac Second-epoch detections are separated by 0.7" and 7.4 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 J336.2954+41.1964 | 22:25:10.92 +41:11:47.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:10.79 +41:11:46.2: 13.23 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:10.79 +41:11:46.2: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 J336.2954+41.1964,2461185.8473,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.2954+41.1964 20260525.3473 9.89CV 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 25.3473 2461185.8473 9.92 22:25:57.18 +40:25:48.2
95.14550 -14.46383 galactic Lac Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 1" Gaia DR3 1909345239202533120
Type: ROT
# Max. Min./Amp. JD0 Period
12.160 G 12.190 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:57.18 +40:25:48.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:57.18 +40:25:48.2: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 1909345239202533120,2461185.8473,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1909345239202533120 20260525.3473 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3473 2461185.8473 9.65 22:23:00.35 +33:22:31.9
90.51176 -19.99054 galactic Peg Second-epoch detections are separated by 0.3" and 7.6 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 1902144327094668416 | 22:23:00.34 +33:22:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:00.35 +33:22:31.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:00.35 +33:22:31.9: 12.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 1902144327094668416,2461185.8473,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1902144327094668416 20260525.3473 9.65CV 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 25.3473 2461185.8473 10.00 22:24:01.20 +39:08:02.8
94.08774 -15.34277 galactic Lac Second-epoch detections are separated by 1.6" and 7.4 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 J336.0052+39.1345 | 22:24:01.27 +39:08:04.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.526+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:01.20 +39:08:02.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:01.20 +39:08:02.8: 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 J336.0052+39.1345,2461185.8473,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.0052+39.1345 20260525.3473 10.00CV 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 25.3473 2461185.8473 10.06 22:26:30.26 +42:15:27.1
96.25542 -12.98468 galactic Lac Second-epoch detections are separated by 0.6" and 7.4 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 J336.6264+42.2578 | 22:26:30.35 +42:15:28.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:30.26 +42:15:27.1: 11.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:30.26 +42:15:27.1: 13.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 J336.6264+42.2578,2461185.8473,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.6264+42.2578 20260525.3473 10.06CV 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 25.3473 2461185.8473 10.09 22:25:02.35 +38:38:36.5
93.97787 -15.86129 galactic Lac Second-epoch detections are separated by 0.9" and 7.4 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 J336.2601+38.6437 | 22:25:02.44 +38:38:37.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.649+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:02.35 +38:38:36.5: 13.06 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:02.35 +38:38:36.5: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 J336.2601+38.6437,2461185.8473,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.2601+38.6437 20260525.3473 10.09CV 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 25.3473 2461185.8473 10.03 22:27:43.44 +38:34:06.4
94.39171 -16.21136 galactic Lac Second-epoch detections are separated by 1.1" and 7.5 pix
The object was found in VSX 2" Gaia DR3 1908595063034286336
Type: VAR
# Max. Min./Amp. JD0 Period
12.270 G 12.320 G 0.015632200000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:43.44 +38:34:06.4: 12.92 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:43.44 +38:34:06.4: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 1908595063034286336,2461185.8473,10.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1908595063034286336 20260525.3473 10.03CV 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 25.3473 2461185.8473 9.44 22:27:00.92 +41:35:40.0
95.96992 -13.59420 galactic Lac Second-epoch detections are separated by 0.2" and 7.4 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 J336.7543+41.5948 | 22:27:01.06 +41:35:41.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.653+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:00.92 +41:35:40.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:00.92 +41:35:40.0: 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
ATO J336.7543+41.5948,2461185.8473,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.7543+41.5948 20260525.3473 9.44CV 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 25.3473 2461185.8473 10.21 22:22:34.15 +40:52:05.2
94.84087 -13.74511 galactic Lac Second-epoch detections are separated by 0.6" and 7.4 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 J335.6455+40.8684 | 22:22:34.21 +40:52:06.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.739+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:34.15 +40:52:05.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:34.15 +40:52:05.2: 13.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 J335.6455+40.8684,2461185.8473,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.6455+40.8684 20260525.3473 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 25.3473 2461185.8473 10.16 22:22:30.47 +41:47:35.7
95.35719 -12.96815 galactic Lac Second-epoch detections are separated by 0.9" and 7.3 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 1957714675556167040 | 22:22:30.53 +41:47:36.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.718+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:22:30.47 +41:47:35.7: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:22:30.47 +41:47:35.7: 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
Gaia DR3 1957714675556167040,2461185.8473,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957714675556167040 20260525.3473 10.16CV 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 25.3473 2461185.8473 10.29 22:27:09.21 +40:20:16.7
95.29210 -14.66535 galactic Lac Second-epoch detections are separated by 1.2" and 7.4 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 | 22:27:09.21 +40:20:16.7 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:09.21 +40:20:16.7: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:09.21 +40:20:16.7: 13.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461185.8473,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.29CV 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 25.3473 2461185.8473 10.04 22:29:17.65 +41:28:02.2
96.27032 -13.93024 galactic Lac Second-epoch detections are separated by 0.1" and 7.4 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 J337.3237+41.4676 | 22:29:17.70 +41:28:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:17.65 +41:28:02.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:17.65 +41:28:02.2: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 J337.3237+41.4676,2461185.8473,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J337.3237+41.4676 20260525.3473 10.04CV 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 25.3473 2461185.8473 10.33 22:25:38.23 +42:04:05.8
96.01159 -13.05682 galactic Lac Second-epoch detections are separated by 1.1" and 7.3 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 | 22:25:38.23 +42:04:05.8 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:25:38.23 +42:04:05.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:25:38.23 +42:04:05.8: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 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,2461185.8473,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 9.99 22:23:37.34 +38:47:39.1
93.82544 -15.58279 galactic Lac Second-epoch detections are separated by 0.2" and 7.4 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 1908734112598757632 | 22:23:37.45 +38:47:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.723+/-0.024 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:37.34 +38:47:39.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:37.34 +38:47:39.1: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 1908734112598757632,2461185.8473,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1908734112598757632 20260525.3473 9.99CV 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 25.3473 2461185.8473 10.29 22:27:53.50 +39:12:46.3
94.78405 -15.68788 galactic Lac Second-epoch detections are separated by 0.4" and 7.5 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 | 22:27:53.50 +39:12:46.3 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.030 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:53.50 +39:12:46.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:53.50 +39:12:46.3: 13.29 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461185.8473,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.29CV 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 25.3473 2461185.8473 10.28 22:21:42.26 +40:38:49.2
94.57416 -13.83794 galactic Lac Second-epoch detections are separated by 0.6" and 7.3 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 J335.4237+40.6505 | 22:21:42.37 +40:38:50.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.793+/-0.026 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:42.26 +40:38:49.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:42.26 +40:38:49.2: 13.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 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 J335.4237+40.6505,2461185.8473,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.4237+40.6505 20260525.3473 10.28CV 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 25.3473 2461185.8473 10.12 22:21:12.77 +33:36:39.2
90.32980 -19.58333 galactic Peg Second-epoch detections are separated by 0.7" and 7.6 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 J335.3032+33.6129 | 22:21:12.77 +33:36:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.029 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:12.77 +33:36:39.2: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:12.77 +33:36:39.2: 13.24 +/- 0.06 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
ATO J335.3032+33.6129,2461185.8473,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J335.3032+33.6129 20260525.3473 10.12CV 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 25.3473 2461185.8473 10.32 22:26:23.92 +39:12:21.1
94.52815 -15.53639 galactic Lac Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 2" Gaia DR3 1908672750402617600
Type: VAR
# Max. Min./Amp. JD0 Period
12.570 G 17.530 G 0.041685100000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:23.92 +39:12:21.1: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:23.92 +39:12:21.1: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 1908672750402617600,2461185.8473,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1908672750402617600 20260525.3473 10.32CV 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 25.3473 2461185.8473 10.52 22:23:32.73 +35:41:57.4
92.00337 -18.13990 galactic Lac Second-epoch detections are separated by 0.3" and 7.5 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 | 22:23:32.73 +35:41:57.4 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.026 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:32.73 +35:41:57.4: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:32.73 +35:41:57.4: 13.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461185.8473,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.52CV 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 25.3473 2461185.8473 10.43 22:23:50.38 +40:10:59.7
94.65780 -14.44923 galactic Lac Second-epoch detections are separated by 0.9" and 7.5 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 | ZTF DR3 | 22:23:50.38 +40:10:59.7 (user input) | 733107200022972 (VSX @ VizieR) | RR: (VSX @ VizieR) | (position from user input) J-Ks=0.289+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:23:50.38 +40:10:59.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:23:50.38 +40:10:59.7: 13.29 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.29 +/- 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
ZTF DR3,2461185.8473,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 DR3 20260525.3473 10.43CV 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 25.3473 2461185.8473 10.53 22:21:09.27 +38:20:25.4
93.14659 -15.68897 galactic Lac Second-epoch detections are separated by 0.9" and 7.4 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 | 22:21:09.27 +38:20:25.4 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:09.27 +38:20:25.4: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:09.27 +38:20:25.4: 13.38 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 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,2461185.8473,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 10.65 22:24:14.06 +41:20:03.0
95.37456 -13.52919 galactic Lac Second-epoch detections are separated by 1.8" and 7.3 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 | 22:24:14.06 +41:20:03.0 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:14.06 +41:20:03.0: 12.89 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:14.06 +41:20:03.0: 13.53 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461185.8473,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.65CV 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 25.3473 2461185.8473 10.53 22:26:22.35 +40:13:20.3
95.09787 -14.68161 galactic Lac Second-epoch detections are separated by 1.1" and 7.5 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 | 22:26:22.35 +40:13:20.3 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.031 (F)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:26:22.35 +40:13:20.3: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:26:22.35 +40:13:20.3: 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
target,2461185.8473,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 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 25.3473 2461185.8473 10.54 22:24:21.88 +37:53:04.8
93.42584 -16.41998 galactic Lac Second-epoch detections are separated by 0.5" and 7.5 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 | 22:24:21.88 +37:53:04.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:21.88 +37:53:04.8: 12.19 +/- 0.11 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:21.88 +37:53:04.8: 13.60 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.16 +/- 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,2461185.8473,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.54CV 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 25.3473 2461185.8473 10.60 22:27:32.23 +40:12:33.7
95.28375 -14.81310 galactic Lac Second-epoch detections are separated by 0.4" and 7.4 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 | 22:27:32.23 +40:12:33.7 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:27:32.23 +40:12:33.7: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:27:32.23 +40:12:33.7: 13.65 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461185.8473,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.60CV 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 25.3473 2461185.8473 10.63 22:28:36.87 +41:59:19.8
96.44629 -13.42145 galactic Lac Second-epoch detections are separated by 0.9" and 7.4 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 | Large-amplitude variable Gaia DR2 1957584147205428224 | 22:28:36.87 +41:59:19.8 (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=0.685+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:36.87 +41:59:19.8: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:36.87 +41:59:19.8: 13.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 1957584147205428224,2461185.8473,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957584147205428224 20260525.3473 10.63CV 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 25.3473 2461185.8473 10.19 22:24:47.79 +41:23:34.1
95.49837 -13.53787 galactic Lac Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX12" Gaia DR3 1957496181979308928
Type: ROT
# Max. Min./Amp. JD0 Period
17.560 G 17.680 G 1.961320000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:47.79 +41:23:34.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:47.79 +41:23:34.1: 13.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 1957496181979308928,2461185.8473,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957496181979308928 20260525.3473 10.19CV 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 25.3473 2461185.8473 10.58 22:21:24.83 +40:44:14.1
94.57889 -13.73232 galactic Lac Second-epoch detections are separated by 0.8" and 7.3 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 | 22:21:24.83 +40:44:14.1 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:21:24.83 +40:44:14.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:21:24.83 +40:44:14.1: 13.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 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,2461185.8473,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3473 10.58CV 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 25.3473 2461185.8473 10.55 22:24:29.96 +39:20:53.4
94.29055 -15.21565 galactic Lac Second-epoch detections are separated by 0.4" and 7.4 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 J336.1210+39.3495 | 22:24:29.96 +39:20:53.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.606+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:24:29.96 +39:20:53.4: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:24:29.96 +39:20:53.4: 13.56 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 J336.1210+39.3495,2461185.8473,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J336.1210+39.3495 20260525.3473 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 25.3473 2461185.8473 10.68 22:29:26.94 +40:50:02.5
95.94736 -14.48145 galactic Lac Second-epoch detections are separated by 1.1" and 7.6 pix
The object was found in VSX 2" Gaia DR3 1909417806969836544
Type: ROT
# Max. Min./Amp. JD0 Period
12.780 G 12.800 G 24.604000000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:29:26.94 +40:50:02.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:29:26.94 +40:50:02.5: 13.60 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 1909417806969836544,2461185.8473,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1909417806969836544 20260525.3473 10.68CV 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 25.3473 2461185.8473 9.46 22:28:16.73 +41:56:38.2
96.36740 -13.42603 galactic Lac Second-epoch detections are separated by 2.8" and 7.7 pix
The object was found in VSX25" Gaia DR3 1957578134253911808
Type: E
# Max. Min./Amp. JD0 Period
19.350 G 19.910 G 0.248229000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:28:16.73 +41:56:38.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:28:16.73 +41:56:38.2: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 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 1957578134253911808,2461185.8473,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1957578134253911808 20260525.3473 9.46CV 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 25.3473 2461185.8473 8.74 22:18:47.95 +40:40:39.3
94.12259 -13.50337 galactic Lac Second-epoch detections are separated by 0.1" and 7.3 pix
The object was found in VSX 2" FV Lac
Type: M
# Max. Min./Amp. JD0 Period
13.000 pg < 15.500 pg 2436860.00000 198.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:18:47.95 +40:40:39.3: 13.44 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:18:47.95 +40:40:39.3: 13.15 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 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
FV Lac,2461185.8473,8.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FV Lac 20260525.3473 8.74CV 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 25.3473 2461185.8473 11.22 22:19:47.33 +42:24:09.0
95.27475 -12.18133 galactic Lac Second-epoch detections are separated by 3.9" and 7.6 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 1958532853945554816 | 22:19:45.71 +42:23:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:19:47.33 +42:24:09.0: 13.23 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q1b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:19:47.33 +42:24:09.0: 13.89 +/- 0.12 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
Gaia DR3 1958532853945554816,2461185.8473,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1958532853945554816 20260525.3473 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
## 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-Q1b1x1_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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461185.84761228 25.05.2026 08:20:23.701 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q1b1x1_033929_TTUQ1b1x1_3226133_znNLp9oG/fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 152
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: 26 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): 28273
Objects passed selection criteria: 28256
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 26432.8
Average stars matched: 25470 (96.3577 %)
Memory usage VmPeak: 130836 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 04:30:27 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-Q1b1x1_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-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461185.84761228 25.05.2026 08:20:23.701 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cyg-07-Q1b1x1_033929_TTUQ1b1x1_3226133_znNLp9oG/fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 826
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 211 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): 163372
Objects passed selection criteria: 163069
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 156640
Average stars matched: 153242 (97.8305 %)
Memory usage VmPeak: 1954352 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 04:37:44 CDT 2026
Host name: tau
############################################################
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Considering the candidate 31047_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31047_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31049_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31049_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31054_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31054_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31104_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31104_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:51.59 +33:03:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31149_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31149_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:48.26 +33:15:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31197_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31197_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:25:45.61 +38:49:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31232_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31232_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31236_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31236_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:31:14.95 +38:46:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 1.876 1964379403950450560 322.81239217790 +38.77559847284 12.1472 10.2801 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31268_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31268_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:14:57.30 +38:02:07.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31301_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31301_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:28.45 +34:14:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31306_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31306_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:09:17.45 +42:22:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31309_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31309_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:15:54.59 +38:11:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31317_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31317_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:27:25.87 +37:08:07.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31319_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31319_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:21:01.06 +40:03:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31321_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31321_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31323_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31323_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:54:17.01 +42:38:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31331_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31331_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31352_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31352_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31357_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31357_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31358_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31358_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31359_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31359_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31361_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31361_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31364_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31364_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31366_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31366_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31369_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31369_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:11:28.18 +35:37:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31370_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31370_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31375_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31375_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31383_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31383_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31387_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31387_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31388_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31388_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31391_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31391_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31393_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31393_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31395_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31395_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:26:52.26 +41:39:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31400_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31400_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31401_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31401_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31402_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31402_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31403_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31403_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31411_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31411_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31412_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31412_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:18:30.78 +41:07:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31413_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31413_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31415_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31415_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31416_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31416_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:44:27.62 +40:44:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31418_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31418_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31421_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31421_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31424_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31424_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31430_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31430_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31432_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31432_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31435_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31435_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31437_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31437_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31439_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31439_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31441_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31441_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31442_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31442_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31445_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31445_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31446_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31446_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:23.26 +41:36:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31450_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31450_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31451_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31451_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31453_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31453_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31454_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31454_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31455_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31455_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31456_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31456_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31458_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31458_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31463_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31463_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31464_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31464_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31465_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31465_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31466_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31466_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31468_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31468_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31469_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31469_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31471_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31471_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31472_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31472_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31473_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31473_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31475_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31475_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31476_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31476_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31477_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31477_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31479_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31479_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31480_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31480_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31481_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31481_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31484_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31484_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31486_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31486_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31487_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31487_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31489_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31489_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31494_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31494_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31497_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31497_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31499_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31499_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31500_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31500_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31501_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31501_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:01:52.31 +40:32:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31504_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31504_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31507_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31507_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31515_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31515_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31517_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31517_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31518_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31518_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31521_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31521_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31522_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31522_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31523_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31523_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31524_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31524_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31528_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31528_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31529_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31529_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31530_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31530_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31533_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31533_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31534_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31534_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31536_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31536_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31537_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31537_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31538_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31538_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31541_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31541_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31543_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31543_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31545_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31545_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31546_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31546_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31547_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31547_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31549_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31549_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31550_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31550_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31551_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31551_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31552_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31552_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31553_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31553_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31558_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31558_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31560_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31560_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31561_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31561_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31562_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31562_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31567_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31567_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31575_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31575_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31576_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31576_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31577_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31577_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31578_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31578_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31582_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31582_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31586_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31586_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31590_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31590_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31595_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31595_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31596_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31596_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31602_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31602_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31611_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31611_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31613_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31613_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31619_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31619_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31629_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31629_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31640_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31640_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31646_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31646_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31653_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31653_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31675_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31675_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 31738_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 31738_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 30137_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 30137_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:27:05.12 +39:40:19.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30097_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 30097_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 02912_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 02912_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 218220_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218220_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218222_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218222_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218223_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218223_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218224_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218224_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218229_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218229_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218234_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218234_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218235_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218235_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218240_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218240_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218250_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218250_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218251_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218251_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218253_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218253_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218256_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218256_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218262_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218262_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218263_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218263_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218269_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218269_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218270_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218270_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218271_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218271_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218275_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218275_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218276_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218276_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218280_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218280_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218288_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218288_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218290_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218290_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218297_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218297_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218298_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218298_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218307_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218307_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218314_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218314_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218316_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218316_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218319_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218319_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218322_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218322_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218323_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218323_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218325_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218325_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218326_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218326_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 218327_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218327_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218328_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218328_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218334_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218334_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218336_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218336_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218337_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218337_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218341_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218341_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218342_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218342_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218343_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218343_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 218345_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218345_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218348_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218348_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218349_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218349_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218350_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218350_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218354_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218354_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218356_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218356_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218358_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218358_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218360_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218360_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:11:17.53 +34:21:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218365_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218365_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218366_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218366_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 218374_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218374_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218377_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218377_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218378_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218378_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218379_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218379_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218380_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218380_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218385_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218385_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218386_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218386_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218387_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218387_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218388_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218388_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218390_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218390_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:13:51.87 +36:05:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218393_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218393_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218394_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218394_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218396_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218396_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218398_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218398_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 218399_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218399_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218402_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218402_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218407_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218407_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:13:42.45 +37:57:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218408_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218408_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218410_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218410_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218411_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218411_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218416_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218416_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218417_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218417_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218418_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218418_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218419_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218419_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218423_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218423_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218424_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218424_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218427_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218427_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218429_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218429_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218430_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218430_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218434_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218434_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218435_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218435_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:20:54.47 +38:29:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218436_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218436_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218437_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218437_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218438_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218438_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218441_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218441_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:22:03.54 +37:55:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218442_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218442_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218443_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218443_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218447_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218447_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:15:14.77 +35:09:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218449_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218449_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218453_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218453_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218454_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218454_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218455_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218455_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218456_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218456_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218458_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218458_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:14:21.97 +35:25:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218461_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218461_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218464_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218464_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:13:41.40 +33:18:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218466_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218466_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218469_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218469_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218470_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218470_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218471_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218471_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 218475_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218475_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:16:17.89 +33:36:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218477_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218477_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218480_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218480_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218481_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218481_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218514_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218514_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:28.10 +34:19:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:46.56 +33:22:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218536_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218536_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:51.55 +33:03:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218559_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218559_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218580_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218580_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:48.29 +33:15:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218674_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218674_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:09:24.99 +39:11:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218684_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218684_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218735_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218735_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:28.41 +34:14:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218745_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218745_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218750_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218750_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218781_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218781_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:14:25.86 +34:53:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218827_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218827_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:23:22.07 +42:04:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218902_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218902_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 218947_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218947_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 218969_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218969_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:31:53.49 +41:44:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218984_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 218984_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:47:14.32 +41:48:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218995_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 218995_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219006_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219006_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219015_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219015_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219052_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219052_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219055_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219055_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:09:40.80 +42:24:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219059_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219059_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219089_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219089_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219121_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219121_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:12:19.72 +40:08:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219138_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219138_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219172_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219172_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219212_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219212_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:12:56.56 +34:25:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219220_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219220_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219252_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219252_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219287_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219287_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219313_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219313_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219345_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219345_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:11:02.10 +38:21:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219420_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219420_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219421_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219421_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219423_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219423_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219442_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219442_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:20:11.13 +39:11:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219476_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219476_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219520_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219520_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219553_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219553_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219570_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219570_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219571_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219571_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219578_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219578_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219640_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219640_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219651_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219651_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219656_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219656_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219660_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219660_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:09:38.21 +40:37:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219665_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219665_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219690_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219690_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:10:53.95 +34:42:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219694_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219694_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219708_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219708_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:20:36.65 +35:06:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219710_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219710_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219723_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219723_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219735_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219735_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 219748_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219748_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219784_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219784_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219804_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219804_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219824_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219824_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219832_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219832_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:20:42.16 +40:40:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219851_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219851_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219853_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219853_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219865_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219865_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219872_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219872_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219874_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219874_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219876_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219876_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219885_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219885_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219889_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219889_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219890_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219890_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:15:01.76 +41:23:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219904_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219904_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:26:16.30 +42:17:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219915_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219915_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219917_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219917_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219934_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219934_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 219953_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219953_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:08:52.59 +41:16:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219965_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219965_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219968_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219968_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219970_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219970_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219976_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219976_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 219977_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 219977_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:13:33.23 +36:38:22.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 219992_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 219992_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220002_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220002_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220016_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220016_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220027_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220027_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220028_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220028_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220030_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220030_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220033_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220033_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220041_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220041_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220042_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220042_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220082_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220082_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:20:24.72 +37:37:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220094_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220094_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220103_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220103_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220114_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220114_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:25:08.70 +42:50:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220115_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220115_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:15:13.83 +42:58:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220130_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220130_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220136_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220136_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220138_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220138_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220163_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220163_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220173_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220173_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220184_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220184_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220204_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220204_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220205_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220205_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220227_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220227_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220236_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220236_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220244_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220244_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220256_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220256_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:07:24.26 +42:31:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220264_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220264_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220271_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220271_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220278_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220278_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220282_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220282_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220283_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220283_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220293_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220293_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220302_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220302_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220313_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220313_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220317_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220317_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220320_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220320_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:07:26.39 +42:30:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220326_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220326_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220334_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220334_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220337_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220337_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220366_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220366_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:55:01.52 +42:15:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220368_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220368_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220376_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220376_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220378_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220378_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220391_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220391_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220400_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220400_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220404_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220404_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:26:22.89 +41:22:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220406_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220406_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220407_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220407_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:38:17.65 +42:07:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220420_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220420_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220425_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220425_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220427_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220427_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220430_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220430_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:30:27.89 +41:53:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220433_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220433_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220451_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220451_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220458_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220458_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220464_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220464_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220473_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220473_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220474_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220474_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:49:46.89 +41:07:51.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 220491_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220491_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220494_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220494_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220502_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220502_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220508_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220508_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220513_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220513_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220515_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220515_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220516_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220516_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220527_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220527_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220540_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220540_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220546_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220546_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220547_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220547_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220549_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220549_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220551_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220551_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220559_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220559_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:30:39.90 +41:59:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220562_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220562_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220564_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220564_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220569_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220569_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:09:33.53 +41:54:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220580_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220580_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220582_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220582_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220586_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220586_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220588_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220588_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220594_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220594_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220599_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220599_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220602_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220602_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220603_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220603_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220609_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220609_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220613_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220613_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220620_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220620_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:43:17.50 +42:44:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220623_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220623_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220625_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220625_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220629_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220629_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220632_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220632_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220641_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220641_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220650_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220650_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220652_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220652_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220654_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220654_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220656_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220656_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220658_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220658_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220662_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220662_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220666_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220666_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220679_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220679_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220683_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220683_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220688_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220688_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220693_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220693_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220694_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220694_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220702_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220702_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220706_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220706_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220711_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220711_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220713_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220713_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220718_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220718_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220719_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220719_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220720_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220720_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220727_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220727_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220731_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220731_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220732_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220732_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220740_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220740_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220743_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220743_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:08:45.34 +42:44:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220745_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220745_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220752_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220752_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220759_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220759_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220760_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220760_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220769_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220769_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220777_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220777_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220781_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220781_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220783_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220783_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220797_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220797_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220802_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220802_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220805_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220805_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220814_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220814_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220818_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220818_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220823_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220823_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220824_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220824_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220829_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220829_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220831_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220831_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220835_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220835_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220837_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220837_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220842_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220842_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220843_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220843_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220845_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220845_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220851_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220851_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220867_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220867_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220868_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220868_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220875_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220875_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220887_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220887_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220889_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220889_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:17:33.40 +35:22:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220916_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220916_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220919_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220919_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220930_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220930_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:56:35.09 +42:36:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220933_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220933_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220934_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220934_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220936_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220936_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220938_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220938_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220944_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220944_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220946_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220946_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220952_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220952_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220956_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220956_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220957_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220957_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 220962_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220962_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220964_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220964_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220966_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220966_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220968_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220968_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220969_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220969_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220970_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220970_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220981_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220981_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220985_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220985_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220987_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 220987_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 220999_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 220999_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221000_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221000_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221004_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221004_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221021_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221021_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221022_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221022_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221027_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221027_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221029_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221029_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221032_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221032_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221034_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221034_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221036_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221036_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221037_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221037_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221039_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221039_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221040_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221040_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:09:22.93 +42:19:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221042_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221042_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221047_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221047_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221048_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221048_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221050_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221050_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221057_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221057_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221062_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221062_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221066_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221066_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221068_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221068_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221070_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221070_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221071_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221071_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221074_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221074_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221077_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221077_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221080_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221080_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221084_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221084_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221086_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221086_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221090_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221090_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221092_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221092_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221093_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221093_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221097_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221097_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221099_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221099_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221100_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221100_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221102_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221102_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221103_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221103_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221106_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221106_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221116_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221116_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221120_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221120_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221122_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221122_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221124_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221124_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221129_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221129_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221137_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221137_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221138_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221138_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221140_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221140_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221149_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221149_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221150_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221150_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221153_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221153_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221154_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221154_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221155_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221155_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221157_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221157_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221158_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221158_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221162_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221162_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221170_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221170_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221171_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221171_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221172_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221172_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221176_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221176_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221177_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221177_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221179_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221179_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221185_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221185_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221189_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221189_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221194_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221194_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221196_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221196_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221197_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221197_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221199_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221199_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221201_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221201_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221206_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221206_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221218_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221218_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221219_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221219_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221226_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221226_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221228_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221228_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221230_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221230_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221235_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221235_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221244_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221244_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221246_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221246_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221248_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221248_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221249_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221249_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221252_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221252_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221253_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221253_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221255_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221255_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221260_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221260_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221263_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221263_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221272_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221272_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221275_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221275_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221286_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221286_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221289_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221289_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221294_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221294_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221296_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221296_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221305_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221305_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221329_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221329_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221335_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221335_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 221341_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221341_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221349_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221349_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221362_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221362_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221368_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221368_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221372_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221372_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221378_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221378_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221382_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221382_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221385_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221385_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221388_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221388_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221392_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221392_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221395_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221395_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221396_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221396_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221397_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221397_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221401_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221401_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221403_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221403_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 221408_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221408_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221412_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221412_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221416_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221416_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221419_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221419_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:44:52.61 +41:26:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221420_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221420_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 221422_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221422_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221425_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221425_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221426_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221426_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221428_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221431_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221431_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221440_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221440_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221441_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221441_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221447_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221447_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221448_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221448_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221450_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221450_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221466_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221466_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221468_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221468_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221472_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221472_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221473_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221473_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221474_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221474_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221479_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221479_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221481_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221481_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221484_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221484_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221486_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221486_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221489_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221489_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221492_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221492_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221493_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221493_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221498_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221498_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221499_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221499_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221503_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221503_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221506_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221506_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221508_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221508_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221518_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221518_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221519_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221519_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221522_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221522_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221525_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221525_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221529_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221529_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221536_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221536_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 221545_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221545_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221546_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221546_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221553_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221553_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221559_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221559_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221563_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221563_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221579_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221579_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221581_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221581_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221584_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221584_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221585_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221585_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221586_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221586_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221588_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221588_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221589_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221589_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221596_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221596_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221597_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221597_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221598_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221598_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221610_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221610_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221611_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221611_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221615_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221615_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221621_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221621_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221624_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221624_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221625_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221625_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221628_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221628_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221630_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221630_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221634_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221634_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221640_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221640_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221643_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221643_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 221651_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221651_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221654_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221654_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221656_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221656_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221659_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221659_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221668_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221668_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221673_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221673_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221674_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221674_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221675_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221675_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221677_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221677_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221686_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221686_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221690_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221690_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221692_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221692_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221695_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221695_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221700_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221700_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221701_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221701_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221704_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221704_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221709_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221709_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221712_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221712_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221713_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221713_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221714_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221714_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221721_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221721_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221728_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221728_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221735_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221735_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221737_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221737_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221743_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221743_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221746_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221746_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221747_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221747_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 221748_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221748_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221753_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221753_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221757_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221757_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221761_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221761_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221773_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221773_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221783_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221783_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221784_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221784_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221787_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 221787_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 221788_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221788_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221790_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221790_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221799_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221799_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221801_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221801_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221807_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221807_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221808_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221808_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221812_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221812_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221814_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221814_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221816_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221816_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221820_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221820_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221823_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221823_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221827_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221827_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221829_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221829_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221831_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221831_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221834_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221834_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221837_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221837_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221838_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221838_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221840_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221840_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221844_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221844_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221845_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221845_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221849_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221849_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221861_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221861_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221862_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221862_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221864_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221864_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221869_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221869_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221870_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221870_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221872_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221872_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221874_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221874_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221876_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221876_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221882_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221882_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221894_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221894_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221897_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221897_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221900_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221900_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221902_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221902_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221906_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221906_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221924_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221924_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221932_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221932_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221934_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221934_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221944_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221944_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221949_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221949_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221952_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221952_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221958_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221958_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221959_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221959_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221966_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221966_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221968_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221968_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221973_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221973_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221979_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221979_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221981_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221981_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221985_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221985_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221987_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221987_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 221999_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 221999_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222007_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 222007_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 222023_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222023_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222024_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222024_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222027_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222027_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222031_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222031_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222032_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 222032_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 222037_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222037_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222044_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222044_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222050_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 222050_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 222064_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222064_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222071_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222071_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222076_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222076_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222089_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222089_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222099_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222099_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222111_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222111_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222125_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222125_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222129_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222129_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222134_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222134_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222140_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222140_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222142_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222142_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222146_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222146_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222156_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 222156_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 222180_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222180_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222182_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222182_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 222186_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 222186_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 161759_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 161759_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212518_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212518_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213133_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213133_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213502_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 213502_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:28:13.51 +39:21:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31424_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 31424_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 154652_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 154652_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 35840_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 35840_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 19230_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 19230_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 157189_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 157189_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 158744_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 158744_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 52132_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 52132_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 175664_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 175664_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 76861_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 76861_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 33331_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 33331_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:26:52.22 +41:39:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158956_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 158956_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 67601_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 67601_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 69343_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 69343_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 89939_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 89939_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 165531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 165531_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 42459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 42459_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:18:30.87 +41:07:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213645_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213645_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213632_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213632_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213526_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213526_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213338_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 213338_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:27:44.69 +39:02:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10756_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 10756_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213251_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 213251_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:25:05.38 +38:56:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213182_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213182_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213161_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213161_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213051_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213051_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213049_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213049_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 213010_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 213010_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212973_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212973_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212964_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212964_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212924_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212924_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212887_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212887_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212795_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212795_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212740_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212740_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 125675_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 125675_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 21:19:07.08 +37:04:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212668_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212668_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212636_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212636_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212611_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212611_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212594_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212594_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212571_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212571_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212550_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212550_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212547_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212547_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212544_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212544_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212538_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212538_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212534_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212534_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212497_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212497_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212439_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212439_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212438_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212438_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212411_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212411_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212408_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212408_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212397_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212397_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212376_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212376_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212326_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212326_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212321_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212321_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212312_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212312_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212270_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212270_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212263_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212263_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212252_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 212252_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
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Considering the candidate 212246_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212246_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212227_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212227_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212219_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212219_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212199_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 212199_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
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Considering the candidate 212143_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 212143_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13745_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 13745_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 44355_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61002_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
The candidate 61002_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357 did not pass the final checks
**** FOUND 22:27:10.64 +39:34:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08741_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
Preparing report for the candidate 08741_fd_Cyg-07-Q1b1x1_2026-05-25_03-20-23_20.00sec_0.00C_LIGHTs_0357
make_report_in_HTML.sh Phase 2 (HTML assembly): 26s
make_report_in_HTML.sh TOTAL: 1345s
Prepared the HTML report for the field Cyg-07-Q1b1x1 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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21:19:12.66 +42:09:19.6
21:20:48.36 +38:04:38.6
21:22:24.73 +38:01:28.6
21:13:13.48 +40:55:44.5
21:33:16.02 +41:46:48.1
21:16:51.47 +38:35:43.6
21:49:04.94 +37:22:34.1
21:28:43.64 +35:42:00.9
21:20:06.71 +36:34:21.2
21:15:57.26 +39:30:06.5
21:31:29.67 +33:55:39.5
21:10:23.61 +41:02:56.4
21:30:05.02 +40:57:00.0
21:24:21.77 +38:05:16.5
21:22:55.49 +41:49:49.9
21:50:40.28 +40:44:27.7
21:16:10.43 +38:43:55.8
21:12:05.84 +40:41:57.5
21:30:39.37 +38:36:13.0
21:16:40.15 +37:19:35.9
21:19:47.74 +36:39:52.8
21:19:40.11 +38:12:51.7
21:14:46.67 +40:23:26.2
21:18:11.75 +41:23:26.2
21:16:03.59 +37:34:29.4
21:11:48.52 +42:10:15.8
21:31:06.80 +39:46:47.2
21:18:56.70 +40:10:47.9
21:28:06.54 +36:36:22.2
21:15:24.90 +41:05:36.9
21:20:28.77 +35:50:51.5
21:11:22.27 +42:02:10.8
21:21:21.34 +38:00:17.5
21:24:31.55 +35:05:22.6
21:15:06.19 +37:57:17.8
22:22:57.31 +41:08:15.2
21:32:05.87 +40:41:03.1
21:17:05.36 +42:12:57.9
21:33:08.65 +41:21:51.9
21:12:36.49 +35:14:51.9
21:46:24.52 +41:13:01.9
21:28:44.93 +38:10:24.2
21:18:22.26 +37:39:43.5
21:19:08.62 +35:54:15.9
21:23:44.88 +38:52:26.7
21:37:50.58 +36:54:52.2
21:38:19.56 +39:47:35.3
22:21:26.07 +42:04:44.1
21:50:17.58 +42:04:56.8
21:23:42.42 +39:12:33.7
21:24:07.47 +35:25:05.5
21:19:21.90 +41:32:54.8
21:17:35.04 +42:45:34.5
21:34:40.18 +37:29:31.8
21:28:43.59 +35:11:00.7
21:43:18.74 +42:12:53.6
21:14:57.38 +39:59:29.7
21:32:16.35 +41:10:14.6
21:13:17.09 +40:02:29.8
21:37:42.98 +40:11:43.1
21:30:38.52 +36:36:07.3
21:12:32.95 +42:38:46.0
21:37:44.49 +42:39:12.3
21:46:20.85 +36:51:37.6
21:44:15.84 +42:45:31.0
21:26:53.39 +40:39:04.3
22:00:32.83 +39:39:03.1
21:20:55.89 +42:02:27.8
21:54:33.42 +35:50:15.0
21:55:49.52 +34:16:12.7
21:58:49.37 +40:28:42.2
21:25:47.96 +38:44:14.8
21:23:15.52 +40:06:52.5
21:21:11.28 +40:12:36.3
21:17:26.71 +36:06:08.9
22:11:18.63 +39:15:04.6
21:38:11.91 +37:42:54.7
21:38:48.53 +41:18:14.6
21:14:03.44 +35:50:46.0
21:41:20.41 +36:37:18.6
21:21:30.19 +39:05:33.9
21:37:02.07 +39:22:40.0
21:29:02.36 +41:37:46.7
21:31:05.87 +41:04:08.3
21:10:16.74 +40:21:12.6
21:53:37.45 +42:42:28.2
21:40:19.37 +35:38:56.5
21:52:16.26 +42:41:08.0
21:24:46.53 +35:05:09.9
21:21:59.18 +39:53:48.7
21:15:04.85 +39:19:08.4
21:13:00.22 +38:06:52.6
21:21:52.77 +34:43:08.5
21:41:27.40 +42:51:23.9
22:00:11.18 +39:37:38.7
21:36:26.19 +42:23:45.7
21:09:49.64 +38:21:37.4
21:14:30.73 +35:31:36.4
21:46:05.72 +42:50:03.3
21:28:40.79 +39:00:17.9
21:45:01.25 +42:15:60.0
21:33:09.21 +37:05:56.5
21:23:39.40 +38:42:01.8
21:35:31.04 +33:55:25.7
21:28:13.70 +33:56:53.8
21:32:31.54 +41:50:58.7
21:32:41.02 +38:29:40.1
21:39:50.83 +41:51:15.2
22:02:09.38 +41:51:02.7
21:55:25.46 +41:56:48.8
21:54:17.19 +36:52:11.4
21:26:28.37 +37:36:33.1
21:21:23.84 +33:48:25.1
21:31:17.20 +37:57:30.7
21:14:45.84 +36:18:04.1
21:24:27.69 +40:15:21.0
22:01:06.44 +42:14:35.8
21:16:12.44 +38:09:29.8
21:28:18.00 +34:05:00.0
21:56:20.29 +42:31:29.4
21:35:50.10 +39:03:54.1
21:33:40.41 +40:44:24.3
21:36:23.84 +37:34:30.9
21:20:02.87 +34:35:15.8
21:46:41.17 +40:55:18.6
21:30:24.45 +39:13:33.0
21:25:22.48 +36:07:15.0
21:49:31.96 +39:23:33.6
21:54:45.67 +38:18:18.0
21:24:23.57 +37:19:36.4
21:21:25.14 +36:00:11.8
22:09:31.96 +42:04:29.4
21:25:13.85 +34:03:17.5
21:32:24.91 +37:04:42.8
21:38:56.76 +37:31:12.5
21:40:15.33 +37:50:20.7
21:39:30.73 +37:21:41.9
22:17:10.57 +41:19:17.1
22:18:25.69 +41:03:50.0
22:18:47.95 +40:40:39.3
22:24:39.80 +40:04:40.5
21:28:06.78 +39:56:16.0
22:24:05.20 +39:13:30.0
22:27:04.57 +38:45:58.5
########### Completed Cyg-07-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:40:23.65 +39:00:27.7
21:35:50.35 +40:48:09.1
21:56:08.18 +40:50:21.0
21:43:42.41 +42:34:57.7
22:06:54.81 +41:38:24.7
21:45:30.06 +40:39:22.2
21:40:19.25 +38:45:41.7
21:32:26.27 +37:28:42.2
21:32:28.08 +38:05:43.0
21:14:40.71 +37:16:07.6
21:29:38.32 +39:05:20.9
21:41:18.31 +41:17:54.2
21:40:47.73 +38:06:20.2
21:19:52.54 +38:04:01.1
21:15:31.73 +38:37:42.4
21:53:19.50 +34:36:59.1
21:28:14.41 +42:51:46.0
21:24:56.62 +36:58:07.4
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21:21:23.82 +41:56:52.4
21:35:24.40 +36:45:52.6
22:09:56.43 +39:05:39.8
21:16:29.78 +36:27:23.2
21:14:58.71 +40:12:43.0
21:30:49.11 +38:57:23.2
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21:46:34.06 +35:50:36.5
22:24:04.86 +41:24:51.1
21:11:00.67 +40:05:05.5
21:28:00.13 +36:42:32.1
21:37:34.51 +32:59:49.5
21:10:29.46 +36:14:17.0
21:25:10.17 +35:57:12.1
21:19:42.35 +38:45:32.1
21:16:57.74 +37:32:50.0
22:23:41.87 +34:37:03.3
22:08:32.91 +35:58:48.5
21:43:35.18 +37:22:30.0
21:27:27.41 +38:09:22.7
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21:36:54.29 +40:36:45.6
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21:24:53.95 +33:31:57.4
21:18:37.33 +33:54:03.0
21:11:57.97 +36:45:24.9
21:50:49.89 +33:01:37.9
21:14:59.46 +34:09:50.9
22:13:08.46 +40:02:52.1
21:17:19.92 +34:34:11.1
22:20:24.64 +41:35:26.1
22:12:22.91 +41:42:04.4
21:25:03.54 +33:29:46.4
22:27:59.83 +41:57:08.5
22:26:53.22 +41:24:28.4
21:16:05.12 +35:26:56.5
21:26:27.74 +35:10:57.9
21:57:39.23 +41:47:19.7
21:11:46.96 +36:20:55.9
21:17:50.23 +39:58:39.7
21:22:48.69 +36:59:03.9
21:40:35.21 +39:13:32.1
21:14:41.88 +36:07:14.6
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22:27:14.92 +42:09:27.2
21:10:46.12 +35:46:39.9
21:09:31.20 +40:48:31.9
21:17:13.96 +41:04:32.0
21:13:58.21 +36:11:59.5
21:12:24.72 +33:36:18.5
21:25:27.48 +37:40:36.4
22:23:06.22 +41:02:00.8
22:20:44.67 +42:23:07.7
21:20:10.14 +33:10:26.1
21:32:48.30 +39:29:39.6
21:21:29.43 +39:04:36.5
21:18:44.62 +36:41:41.9
22:17:24.47 +38:35:02.3
22:28:45.72 +41:44:04.0
21:28:37.89 +35:33:42.3
21:48:46.98 +40:08:13.6
21:18:50.95 +34:56:39.7
21:19:25.52 +34:12:50.4
21:11:10.88 +35:31:16.4
22:28:39.45 +41:36:50.0
21:12:41.04 +33:09:48.9
21:12:13.97 +35:19:19.8
21:17:20.41 +36:43:54.8
21:10:56.05 +35:44:07.0
21:20:25.11 +37:31:57.3
21:21:12.52 +36:20:37.3
21:53:17.43 +42:34:35.4
21:18:26.61 +34:17:33.4
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21:13:16.12 +33:44:29.7
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21:31:14.91 +38:46:29.7
22:29:53.35 +41:26:00.2
21:15:17.47 +38:56:43.3
22:09:13.49 +39:15:45.0
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21:30:37.79 +42:45:58.2
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21:23:35.11 +38:21:41.0
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21:19:37.43 +35:07:20.3
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21:42:06.01 +36:50:53.0
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22:07:49.45 +33:25:38.3
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21:17:59.54 +42:35:34.7
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21:12:49.51 +41:23:27.4
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21:42:46.31 +37:59:49.7
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22:09:21.19 +33:46:49.3
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21:44:49.72 +36:56:53.9
21:21:04.51 +40:28:37.5
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22:24:43.50 +41:45:09.0
21:27:59.74 +37:32:17.8
21:12:46.98 +42:24:03.8
21:14:14.01 +36:03:26.7
21:17:06.42 +35:11:34.0
22:26:17.45 +40:38:22.7
21:42:23.05 +40:36:53.1
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22:02:27.71 +42:04:01.9
21:33:53.13 +33:18:17.1
22:14:09.47 +38:28:27.7
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21:39:02.90 +40:22:35.9
22:05:01.96 +41:27:41.8
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21:18:43.48 +37:57:52.4
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21:50:11.43 +35:33:08.1
21:21:06.53 +36:01:47.5
21:24:57.22 +42:40:16.6
21:11:38.29 +37:30:37.3
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21:39:47.29 +42:43:07.2
21:29:32.10 +33:48:17.3
22:21:24.16 +41:17:43.9
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22:17:25.04 +42:04:44.7
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21:34:59.13 +39:59:54.0
21:09:58.24 +38:52:34.6
21:37:54.69 +33:00:12.4
21:59:59.93 +38:42:23.1
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22:21:51.89 +38:05:41.0
21:56:32.95 +38:17:22.8
21:21:53.02 +41:39:20.3
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21:57:59.24 +41:37:13.3
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21:14:51.36 +38:32:19.8
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21:36:48.43 +38:51:41.5
21:10:24.23 +38:26:35.0
22:04:36.81 +38:54:14.7
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21:20:06.58 +39:26:52.7
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21:11:51.11 +35:37:58.7
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21:11:58.18 +34:50:23.8
21:34:11.25 +40:41:03.1
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21:19:18.15 +42:26:13.0
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21:27:39.99 +41:28:15.9
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21:22:07.42 +37:28:58.6
21:13:30.27 +36:57:14.1
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21:30:06.71 +42:42:51.2
21:09:14.84 +39:51:13.5
21:39:31.73 +40:39:06.9
21:21:45.46 +38:51:10.6
21:14:16.84 +37:13:45.6
21:52:14.88 +36:58:29.7
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21:13:36.47 +40:33:16.4
21:28:24.99 +39:10:02.1
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21:55:49.52 +34:16:12.7
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21:21:11.28 +40:12:36.3
21:17:26.71 +36:06:08.9
22:11:18.63 +39:15:04.6
21:38:11.91 +37:42:54.7
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21:14:03.44 +35:50:46.0
21:41:20.41 +36:37:18.6
21:21:30.19 +39:05:33.9
21:37:02.07 +39:22:40.0
21:29:02.36 +41:37:46.7
21:31:05.87 +41:04:08.3
21:10:16.74 +40:21:12.6
21:53:37.45 +42:42:28.2
21:40:19.37 +35:38:56.5
21:52:16.26 +42:41:08.0
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21:21:59.18 +39:53:48.7
21:15:04.85 +39:19:08.4
21:13:00.22 +38:06:52.6
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21:41:27.40 +42:51:23.9
22:00:11.18 +39:37:38.7
21:36:26.19 +42:23:45.7
21:09:49.64 +38:21:37.4
21:14:30.73 +35:31:36.4
21:46:05.72 +42:50:03.3
21:28:40.79 +39:00:17.9
21:45:01.25 +42:15:60.0
21:33:09.21 +37:05:56.5
21:23:39.40 +38:42:01.8
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21:28:13.70 +33:56:53.8
21:32:31.54 +41:50:58.7
21:32:41.02 +38:29:40.1
21:39:50.83 +41:51:15.2
22:02:09.38 +41:51:02.7
21:55:25.46 +41:56:48.8
21:54:17.19 +36:52:11.4
21:26:28.37 +37:36:33.1
21:21:23.84 +33:48:25.1
21:31:17.20 +37:57:30.7
21:14:45.84 +36:18:04.1
21:24:27.69 +40:15:21.0
22:01:06.44 +42:14:35.8
21:16:12.44 +38:09:29.8
21:28:18.00 +34:05:00.0
21:56:20.29 +42:31:29.4
21:35:50.10 +39:03:54.1
21:33:40.41 +40:44:24.3
21:36:23.84 +37:34:30.9
21:20:02.87 +34:35:15.8
21:46:41.17 +40:55:18.6
21:30:24.45 +39:13:33.0
21:25:22.48 +36:07:15.0
21:49:31.96 +39:23:33.6
21:54:45.67 +38:18:18.0
21:24:23.57 +37:19:36.4
21:21:25.14 +36:00:11.8
22:09:31.96 +42:04:29.4
21:25:13.85 +34:03:17.5
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21:38:56.76 +37:31:12.5
21:40:15.33 +37:50:20.7
21:39:30.73 +37:21:41.9
21:52:59.99 +33:25:12.1
22:25:38.96 +39:59:37.6
22:23:25.16 +41:54:05.1
22:17:10.57 +41:19:17.1
21:57:38.14 +32:57:13.0
22:18:25.69 +41:03:50.0
22:23:57.60 +41:47:31.3
21:12:38.95 +33:09:36.0
22:24:39.80 +40:04:40.5
21:13:52.12 +34:18:26.4
22:27:04.57 +38:45:58.5
21:50:32.90 +33:17:12.9
21:28:06.78 +39:56:16.0
22:24:05.20 +39:13:30.0
22:20:30.72 +33:13:11.8
22:26:47.99 +39:55:16.8
22:27:15.22 +40:20:02.7
22:28:37.12 +40:06:52.2
22:27:39.56 +42:05:42.1
22:27:39.15 +41:18:21.0
22:22:07.59 +40:53:07.5
22:23:44.27 +32:54:14.5
22:12:21.99 +33:37:10.3
22:24:47.11 +40:38:54.7
22:21:42.03 +36:19:16.6
22:25:36.46 +40:51:52.1
22:25:10.79 +41:11:46.2
22:25:57.18 +40:25:48.2
22:23:00.35 +33:22:31.9
22:24:01.20 +39:08:02.8
22:26:30.26 +42:15:27.1
22:25:02.35 +38:38:36.5
22:27:43.44 +38:34:06.4
22:27:00.92 +41:35:40.0
22:22:34.15 +40:52:05.2
22:22:30.47 +41:47:35.7
22:27:09.21 +40:20:16.7
22:29:17.65 +41:28:02.2
22:25:38.23 +42:04:05.8
22:23:37.34 +38:47:39.1
22:27:53.50 +39:12:46.3
22:21:42.26 +40:38:49.2
22:21:12.77 +33:36:39.2
22:26:23.92 +39:12:21.1
22:23:32.73 +35:41:57.4
22:23:50.38 +40:10:59.7
22:21:09.27 +38:20:25.4
22:24:14.06 +41:20:03.0
22:26:22.35 +40:13:20.3
22:24:21.88 +37:53:04.8
22:27:32.23 +40:12:33.7
22:28:36.87 +41:59:19.8
22:24:47.79 +41:23:34.1
22:21:24.83 +40:44:14.1
22:24:29.96 +39:20:53.4
22:29:26.94 +40:50:02.5
22:28:16.73 +41:56:38.2
22:18:47.95 +40:40:39.3
22:19:47.33 +42:24:09.0
###################################################################################
21:40:23.65 +39:00:27.7 -- not an asteroid (will add it to exclusion list)
21:35:50.35 +40:48:09.1 -- not an asteroid (will add it to exclusion list)
21:56:08.18 +40:50:21.0 -- not an asteroid (will add it to exclusion list)
21:43:42.41 +42:34:57.7 -- not an asteroid (will add it to exclusion list)
22:06:54.81 +41:38:24.7 -- not an asteroid (will add it to exclusion list)
21:45:30.06 +40:39:22.2 -- not an asteroid (will add it to exclusion list)
21:40:19.25 +38:45:41.7 -- not an asteroid (will add it to exclusion list)
21:32:26.27 +37:28:42.2 -- not an asteroid (will add it to exclusion list)
21:32:28.08 +38:05:43.0 -- not an asteroid (will add it to exclusion list)
21:14:40.71 +37:16:07.6 -- not an asteroid (will add it to exclusion list)
21:29:38.32 +39:05:20.9 -- not an asteroid (will add it to exclusion list)
21:41:18.31 +41:17:54.2 -- not an asteroid (will add it to exclusion list)
21:40:47.73 +38:06:20.2 -- not an asteroid (will add it to exclusion list)
21:19:52.54 +38:04:01.1 -- not an asteroid (will add it to exclusion list)
21:15:31.73 +38:37:42.4 -- not an asteroid (will add it to exclusion list)
21:53:19.50 +34:36:59.1 -- not an asteroid (will add it to exclusion list)
21:28:14.41 +42:51:46.0 -- not an asteroid (will add it to exclusion list)
21:24:56.62 +36:58:07.4 -- not an asteroid (will add it to exclusion list)
22:08:04.65 +35:52:50.9 -- not an asteroid (will add it to exclusion list)
21:21:23.82 +41:56:52.4 -- not an asteroid (will add it to exclusion list)
21:35:24.40 +36:45:52.6 -- not an asteroid (will add it to exclusion list)
22:09:56.43 +39:05:39.8 -- not an asteroid (will add it to exclusion list)
21:16:29.78 +36:27:23.2 -- not an asteroid (will add it to exclusion list)
21:14:58.71 +40:12:43.0 -- not an asteroid (will add it to exclusion list)
21:30:49.11 +38:57:23.2 -- not an asteroid (will add it to exclusion list)
21:21:41.70 +36:14:58.9 -- not an asteroid (will add it to exclusion list)
21:46:34.06 +35:50:36.5 -- not an asteroid (will add it to exclusion list)
22:24:04.86 +41:24:51.1 -- not an asteroid (will add it to exclusion list)
21:11:00.67 +40:05:05.5 -- not an asteroid (will add it to exclusion list)
21:28:00.13 +36:42:32.1 -- not an asteroid (will add it to exclusion list)
21:37:34.51 +32:59:49.5 -- not an asteroid (will add it to exclusion list)
21:10:29.46 +36:14:17.0 -- not an asteroid (will add it to exclusion list)
21:25:10.17 +35:57:12.1 -- not an asteroid (will add it to exclusion list)
21:19:42.35 +38:45:32.1 -- not an asteroid (will add it to exclusion list)
21:16:57.74 +37:32:50.0 -- not an asteroid (will add it to exclusion list)
22:23:41.87 +34:37:03.3 -- not an asteroid (will add it to exclusion list)
22:08:32.91 +35:58:48.5 -- not an asteroid (will add it to exclusion list)
21:43:35.18 +37:22:30.0 -- not an asteroid (will add it to exclusion list)
21:27:27.41 +38:09:22.7 -- not an asteroid (will add it to exclusion list)
21:16:43.12 +41:35:51.4 -- not an asteroid (will add it to exclusion list)
22:15:54.18 +37:58:56.1 -- not an asteroid (will add it to exclusion list)
21:36:54.29 +40:36:45.6 -- not an asteroid (will add it to exclusion list)
22:24:00.62 +40:01:13.8 -- not an asteroid (will add it to exclusion list)
21:24:53.95 +33:31:57.4 -- not an asteroid (will add it to exclusion list)
21:18:37.33 +33:54:03.0 -- not an asteroid (will add it to exclusion list)
21:11:57.97 +36:45:24.9 -- not an asteroid (will add it to exclusion list)
21:50:49.89 +33:01:37.9 -- not an asteroid (will add it to exclusion list)
21:14:59.46 +34:09:50.9 -- not an asteroid (will add it to exclusion list)
22:13:08.46 +40:02:52.1 -- not an asteroid (will add it to exclusion list)
21:17:19.92 +34:34:11.1 -- not an asteroid (will add it to exclusion list)
22:20:24.64 +41:35:26.1 -- not an asteroid (will add it to exclusion list)
22:12:22.91 +41:42:04.4 -- not an asteroid (will add it to exclusion list)
21:25:03.54 +33:29:46.4 -- not an asteroid (will add it to exclusion list)
22:27:59.83 +41:57:08.5 -- not an asteroid (will add it to exclusion list)
22:26:53.22 +41:24:28.4 -- not an asteroid (will add it to exclusion list)
21:16:05.12 +35:26:56.5 -- not an asteroid (will add it to exclusion list)
21:26:27.74 +35:10:57.9 -- not an asteroid (will add it to exclusion list)
21:57:39.23 +41:47:19.7 -- not an asteroid (will add it to exclusion list)
21:11:46.96 +36:20:55.9 -- not an asteroid (will add it to exclusion list)
21:17:50.23 +39:58:39.7 -- not an asteroid (will add it to exclusion list)
21:22:48.69 +36:59:03.9 -- not an asteroid (will add it to exclusion list)
21:40:35.21 +39:13:32.1 -- not an asteroid (will add it to exclusion list)
21:14:41.88 +36:07:14.6 -- not an asteroid (will add it to exclusion list)
22:01:22.36 +40:55:08.1 -- not an asteroid (will add it to exclusion list)
22:27:14.92 +42:09:27.2 -- not an asteroid (will add it to exclusion list)
21:10:46.12 +35:46:39.9 -- not an asteroid (will add it to exclusion list)
21:09:31.20 +40:48:31.9 -- not an asteroid (will add it to exclusion list)
21:17:13.96 +41:04:32.0 -- not an asteroid (will add it to exclusion list)
21:13:58.21 +36:11:59.5 -- not an asteroid (will add it to exclusion list)
21:12:24.72 +33:36:18.5 -- not an asteroid (will add it to exclusion list)
21:25:27.48 +37:40:36.4 -- not an asteroid (will add it to exclusion list)
22:23:06.22 +41:02:00.8 -- not an asteroid (will add it to exclusion list)
22:20:44.67 +42:23:07.7 -- not an asteroid (will add it to exclusion list)
21:20:10.14 +33:10:26.1 -- not an asteroid (will add it to exclusion list)
21:32:48.30 +39:29:39.6 -- not an asteroid (will add it to exclusion list)
21:21:29.43 +39:04:36.5 -- not an asteroid (will add it to exclusion list)
21:18:44.62 +36:41:41.9 -- not an asteroid (will add it to exclusion list)
22:17:24.47 +38:35:02.3 -- not an asteroid (will add it to exclusion list)
22:28:45.72 +41:44:04.0 -- not an asteroid (will add it to exclusion list)
21:28:37.89 +35:33:42.3 -- not an asteroid (will add it to exclusion list)
21:48:46.98 +40:08:13.6 -- not an asteroid (will add it to exclusion list)
21:18:50.95 +34:56:39.7 -- not an asteroid (will add it to exclusion list)
21:19:25.52 +34:12:50.4 -- not an asteroid (will add it to exclusion list)
21:11:10.88 +35:31:16.4 -- not an asteroid (will add it to exclusion list)
22:28:39.45 +41:36:50.0 -- not an asteroid (will add it to exclusion list)
21:12:41.04 +33:09:48.9 -- not an asteroid (will add it to exclusion list)
21:12:13.97 +35:19:19.8 -- not an asteroid (will add it to exclusion list)
21:17:20.41 +36:43:54.8 -- not an asteroid (will add it to exclusion list)
21:10:56.05 +35:44:07.0 -- not an asteroid (will add it to exclusion list)
21:20:25.11 +37:31:57.3 -- not an asteroid (will add it to exclusion list)
21:21:12.52 +36:20:37.3 -- not an asteroid (will add it to exclusion list)
21:53:17.43 +42:34:35.4 -- not an asteroid (will add it to exclusion list)
21:18:26.61 +34:17:33.4 -- not an asteroid (will add it to exclusion list)
22:01:26.89 +38:07:17.1 -- not an asteroid (will add it to exclusion list)
21:13:16.12 +33:44:29.7 -- not an asteroid (will add it to exclusion list)
22:01:07.92 +39:15:18.7 -- not an asteroid (will add it to exclusion list)
21:31:14.91 +38:46:29.7 -- not an asteroid (will add it to exclusion list)
22:29:53.35 +41:26:00.2 -- not an asteroid (will add it to exclusion list)
21:15:17.47 +38:56:43.3 -- not an asteroid (will add it to exclusion list)
22:09:13.49 +39:15:45.0 -- not an asteroid (will add it to exclusion list)
21:56:49.58 +42:13:05.3 -- not an asteroid (will add it to exclusion list)
21:27:28.52 +35:23:02.6 -- not an asteroid (will add it to exclusion list)
21:30:37.79 +42:45:58.2 -- not an asteroid (will add it to exclusion list)
21:22:36.12 +35:35:48.8 -- not an asteroid (will add it to exclusion list)
21:21:47.77 +35:29:50.0 -- not an asteroid (will add it to exclusion list)
21:26:25.16 +35:51:25.5 -- not an asteroid (will add it to exclusion list)
21:26:53.16 +37:31:50.2 -- not an asteroid (will add it to exclusion list)
21:23:35.11 +38:21:41.0 -- not an asteroid (will add it to exclusion list)
22:02:13.82 +41:47:07.6 -- not an asteroid (will add it to exclusion list)
21:15:42.98 +33:53:35.1 -- not an asteroid (will add it to exclusion list)
22:26:35.03 +36:53:06.5 -- not an asteroid (will add it to exclusion list)
21:24:39.66 +36:58:46.5 -- not an asteroid (will add it to exclusion list)
21:19:37.43 +35:07:20.3 -- not an asteroid (will add it to exclusion list)
22:26:44.89 +40:34:42.4 -- not an asteroid (will add it to exclusion list)
21:14:38.40 +37:33:48.6 -- not an asteroid (will add it to exclusion list)
21:42:06.01 +36:50:53.0 -- not an asteroid (will add it to exclusion list)
21:20:52.17 +38:17:39.5 -- not an asteroid (will add it to exclusion list)
21:25:56.52 +38:11:59.2 -- not an asteroid (will add it to exclusion list)
21:29:08.03 +42:01:02.7 -- not an asteroid (will add it to exclusion list)
22:07:49.45 +33:25:38.3 -- not an asteroid (will add it to exclusion list)
21:14:44.84 +38:12:03.0 -- not an asteroid (will add it to exclusion list)
21:29:04.95 +40:27:04.6 -- not an asteroid (will add it to exclusion list)
21:17:59.54 +42:35:34.7 -- not an asteroid (will add it to exclusion list)
21:26:11.09 +42:43:43.7 -- not an asteroid (will add it to exclusion list)
21:49:54.44 +34:54:43.5 -- not an asteroid (will add it to exclusion list)
22:06:46.45 +39:39:05.9 -- not an asteroid (will add it to exclusion list)
21:12:49.51 +41:23:27.4 -- not an asteroid (will add it to exclusion list)
21:12:50.84 +36:08:07.8 -- not an asteroid (will add it to exclusion list)
21:15:36.32 +36:55:35.8 -- not an asteroid (will add it to exclusion list)
21:42:46.31 +37:59:49.7 -- not an asteroid (will add it to exclusion list)
22:20:30.94 +33:33:35.0 -- not an asteroid (will add it to exclusion list)
22:21:21.34 +41:17:35.6 -- not an asteroid (will add it to exclusion list)
22:09:21.19 +33:46:49.3 -- not an asteroid (will add it to exclusion list)
21:15:25.79 +36:10:50.5 -- not an asteroid (will add it to exclusion list)
21:44:49.72 +36:56:53.9 -- not an asteroid (will add it to exclusion list)
21:21:04.51 +40:28:37.5 -- not an asteroid (will add it to exclusion list)
22:01:57.33 +35:42:30.3 -- not an asteroid (will add it to exclusion list)
22:00:15.47 +42:40:23.2 -- not an asteroid (will add it to exclusion list)
22:24:43.50 +41:45:09.0 -- not an asteroid (will add it to exclusion list)
21:27:59.74 +37:32:17.8 -- not an asteroid (will add it to exclusion list)
21:12:46.98 +42:24:03.8 -- not an asteroid (will add it to exclusion list)
21:14:14.01 +36:03:26.7 -- not an asteroid (will add it to exclusion list)
21:17:06.42 +35:11:34.0 -- not an asteroid (will add it to exclusion list)
22:26:17.45 +40:38:22.7 -- not an asteroid (will add it to exclusion list)
21:42:23.05 +40:36:53.1 -- not an asteroid (will add it to exclusion list)
22:05:53.83 +33:29:13.6 -- not an asteroid (will add it to exclusion list)
22:02:27.71 +42:04:01.9 -- not an asteroid (will add it to exclusion list)
21:33:53.13 +33:18:17.1 -- not an asteroid (will add it to exclusion list)
22:14:09.47 +38:28:27.7 -- not an asteroid (will add it to exclusion list)
21:14:54.60 +34:58:50.3 -- not an asteroid (will add it to exclusion list)
21:16:44.97 +34:40:58.5 -- not an asteroid (will add it to exclusion list)
21:12:59.88 +36:04:17.9 -- not an asteroid (will add it to exclusion list)
21:24:11.07 +37:39:45.7 -- not an asteroid (will add it to exclusion list)
22:17:45.88 +39:00:20.5 -- not an asteroid (will add it to exclusion list)
21:18:02.81 +41:31:39.7 -- not an asteroid (will add it to exclusion list)
21:39:02.90 +40:22:35.9 -- not an asteroid (will add it to exclusion list)
22:05:01.96 +41:27:41.8 -- not an asteroid (will add it to exclusion list)
21:13:09.70 +38:07:24.2 -- not an asteroid (will add it to exclusion list)
21:28:41.55 +42:35:38.9 -- not an asteroid (will add it to exclusion list)
21:26:50.82 +42:27:02.6 -- not an asteroid (will add it to exclusion list)
21:16:35.26 +37:06:18.1 -- not an asteroid (will add it to exclusion list)
21:58:13.38 +38:26:14.2 -- not an asteroid (will add it to exclusion list)
22:15:17.49 +39:47:51.6 -- not an asteroid (will add it to exclusion list)
21:15:47.41 +37:50:42.3 -- not an asteroid (will add it to exclusion list)
21:12:44.35 +36:07:58.7 -- not an asteroid (will add it to exclusion list)
21:18:43.48 +37:57:52.4 -- not an asteroid (will add it to exclusion list)
21:13:16.20 +41:07:40.5 -- not an asteroid (will add it to exclusion list)
22:02:04.51 +37:45:26.1 -- not an asteroid (will add it to exclusion list)
22:05:11.22 +41:31:52.7 -- not an asteroid (will add it to exclusion list)
22:07:43.26 +37:37:03.4 -- not an asteroid (will add it to exclusion list)
21:50:11.43 +35:33:08.1 -- not an asteroid (will add it to exclusion list)
21:21:06.53 +36:01:47.5 -- not an asteroid (will add it to exclusion list)
21:24:57.22 +42:40:16.6 -- not an asteroid (will add it to exclusion list)
21:11:38.29 +37:30:37.3 -- not an asteroid (will add it to exclusion list)
22:12:04.42 +37:38:52.8 -- not an asteroid (will add it to exclusion list)
21:39:47.29 +42:43:07.2 -- not an asteroid (will add it to exclusion list)
21:29:32.10 +33:48:17.3 -- not an asteroid (will add it to exclusion list)
22:21:24.16 +41:17:43.9 -- not an asteroid (will add it to exclusion list)
22:13:03.48 +38:28:18.8 -- not an asteroid (will add it to exclusion list)
22:09:23.69 +40:29:36.8 -- not an asteroid (will add it to exclusion list)
22:17:25.04 +42:04:44.7 -- not an asteroid (will add it to exclusion list)
21:13:58.07 +36:59:38.7 -- not an asteroid (will add it to exclusion list)
21:17:44.76 +38:40:34.1 -- not an asteroid (will add it to exclusion list)
21:17:03.32 +37:35:40.5 -- not an asteroid (will add it to exclusion list)
21:14:34.90 +37:36:52.5 -- not an asteroid (will add it to exclusion list)
21:18:25.07 +38:04:45.1 -- not an asteroid (will add it to exclusion list)
21:34:59.13 +39:59:54.0 -- not an asteroid (will add it to exclusion list)
21:09:58.24 +38:52:34.6 -- not an asteroid (will add it to exclusion list)
21:37:54.69 +33:00:12.4 -- not an asteroid (will add it to exclusion list)
21:59:59.93 +38:42:23.1 -- not an asteroid (will add it to exclusion list)
21:17:15.71 +34:09:14.6 -- not an asteroid (will add it to exclusion list)
22:21:51.89 +38:05:41.0 -- not an asteroid (will add it to exclusion list)
21:56:32.95 +38:17:22.8 -- not an asteroid (will add it to exclusion list)
21:21:53.02 +41:39:20.3 -- not an asteroid (will add it to exclusion list)
22:05:11.01 +42:22:39.9 -- not an asteroid (will add it to exclusion list)
21:42:23.52 +41:49:36.8 -- not an asteroid (will add it to exclusion list)
22:19:20.15 +40:03:19.4 -- not an asteroid (will add it to exclusion list)
21:57:59.24 +41:37:13.3 -- not an asteroid (will add it to exclusion list)
21:19:28.79 +39:57:40.4 -- not an asteroid (will add it to exclusion list)
21:14:51.36 +38:32:19.8 -- not an asteroid (will add it to exclusion list)
21:09:53.82 +42:17:25.4 -- not an asteroid (will add it to exclusion list)
21:11:50.84 +40:34:54.6 -- not an asteroid (will add it to exclusion list)
21:27:09.80 +36:53:13.9 -- not an asteroid (will add it to exclusion list)
22:12:26.42 +40:34:53.0 -- not an asteroid (will add it to exclusion list)
21:14:03.36 +34:52:46.8 -- not an asteroid (will add it to exclusion list)
22:09:11.24 +36:46:05.1 -- not an asteroid (will add it to exclusion list)
21:14:10.55 +37:06:09.0 -- not an asteroid (will add it to exclusion list)
21:36:48.43 +38:51:41.5 -- not an asteroid (will add it to exclusion list)
21:10:24.23 +38:26:35.0 -- not an asteroid (will add it to exclusion list)
22:04:36.81 +38:54:14.7 -- not an asteroid (will add it to exclusion list)
21:37:35.64 +40:12:05.7 -- not an asteroid (will add it to exclusion list)
21:11:38.47 +38:20:47.4 -- not an asteroid (will add it to exclusion list)
21:27:12.32 +39:44:01.5 -- not an asteroid (will add it to exclusion list)
21:12:24.20 +40:10:31.1 -- not an asteroid (will add it to exclusion list)
21:14:41.33 +34:18:39.8 -- not an asteroid (will add it to exclusion list)
21:14:48.66 +37:08:03.6 -- not an asteroid (will add it to exclusion list)
21:20:06.58 +39:26:52.7 -- not an asteroid (will add it to exclusion list)
21:36:15.14 +40:02:53.3 -- not an asteroid (will add it to exclusion list)
21:11:51.11 +35:37:58.7 -- not an asteroid (will add it to exclusion list)
21:18:55.54 +41:30:47.1 -- not an asteroid (will add it to exclusion list)
21:14:40.80 +39:49:56.5 -- not an asteroid (will add it to exclusion list)
21:11:58.18 +34:50:23.8 -- not an asteroid (will add it to exclusion list)
21:34:11.25 +40:41:03.1 -- not an asteroid (will add it to exclusion list)
21:14:07.41 +39:48:24.2 -- not an asteroid (will add it to exclusion list)
21:17:15.26 +35:51:06.5 -- not an asteroid (will add it to exclusion list)
21:29:00.59 +35:14:11.5 -- not an asteroid (will add it to exclusion list)
21:15:07.43 +38:34:26.4 -- not an asteroid (will add it to exclusion list)
21:19:18.15 +42:26:13.0 -- not an asteroid (will add it to exclusion list)
22:01:03.93 +41:04:56.1 -- not an asteroid (will add it to exclusion list)
21:22:28.29 +40:43:48.8 -- not an asteroid (will add it to exclusion list)
21:19:19.25 +39:41:30.2 -- not an asteroid (will add it to exclusion list)
21:56:00.37 +37:10:55.8 -- not an asteroid (will add it to exclusion list)
21:12:39.54 +38:09:44.1 -- not an asteroid (will add it to exclusion list)
21:43:36.58 +42:31:44.2 -- not an asteroid (will add it to exclusion list)
21:11:33.88 +36:22:57.6 -- not an asteroid (will add it to exclusion list)
21:12:04.94 +42:34:05.0 -- not an asteroid (will add it to exclusion list)
21:17:15.27 +41:40:01.8 -- not an asteroid (will add it to exclusion list)
21:26:38.61 +39:47:22.1 -- not an asteroid (will add it to exclusion list)
21:24:42.39 +38:26:36.8 -- not an asteroid (will add it to exclusion list)
21:16:06.05 +38:52:02.3 -- not an asteroid (will add it to exclusion list)
21:16:22.33 +37:47:56.0 -- not an asteroid (will add it to exclusion list)
21:09:04.49 +40:48:05.6 -- not an asteroid (will add it to exclusion list)
21:41:50.86 +35:55:28.9 -- not an asteroid (will add it to exclusion list)
21:46:53.87 +39:15:18.7 -- not an asteroid (will add it to exclusion list)
21:15:45.32 +36:35:09.8 -- not an asteroid (will add it to exclusion list)
21:11:20.88 +39:12:54.3 -- not an asteroid (will add it to exclusion list)
21:12:38.13 +39:31:59.6 -- not an asteroid (will add it to exclusion list)
21:56:34.36 +37:00:25.9 -- not an asteroid (will add it to exclusion list)
21:15:01.14 +37:38:00.8 -- not an asteroid (will add it to exclusion list)
21:19:04.73 +38:33:58.2 -- not an asteroid (will add it to exclusion list)
21:59:30.86 +42:08:23.4 -- not an asteroid (will add it to exclusion list)
21:17:51.46 +37:12:27.1 -- not an asteroid (will add it to exclusion list)
21:13:03.05 +33:40:45.7 -- not an asteroid (will add it to exclusion list)
21:14:26.33 +37:57:13.1 -- not an asteroid (will add it to exclusion list)
21:56:29.02 +36:52:32.3 -- not an asteroid (will add it to exclusion list)
21:35:23.88 +36:47:17.3 -- not an asteroid (will add it to exclusion list)
21:09:56.53 +42:31:27.0 -- not an asteroid (will add it to exclusion list)
21:16:52.19 +40:29:56.3 -- not an asteroid (will add it to exclusion list)
21:17:56.57 +39:27:24.9 -- not an asteroid (will add it to exclusion list)
22:24:31.98 +41:49:20.1 -- not an asteroid (will add it to exclusion list)
21:27:31.59 +35:50:08.1 -- not an asteroid (will add it to exclusion list)
21:18:36.52 +38:08:19.0 -- not an asteroid (will add it to exclusion list)
21:20:37.24 +41:57:32.3 -- not an asteroid (will add it to exclusion list)
21:20:50.00 +33:44:17.2 -- not an asteroid (will add it to exclusion list)
21:11:16.17 +36:08:41.0 -- not an asteroid (will add it to exclusion list)
21:20:39.63 +40:14:13.6 -- not an asteroid (will add it to exclusion list)
21:46:08.61 +35:33:30.2 -- not an asteroid (will add it to exclusion list)
22:26:27.62 +39:49:37.8 -- not an asteroid (will add it to exclusion list)
21:51:38.10 +43:02:19.3 -- not an asteroid (will add it to exclusion list)
21:14:10.79 +37:29:35.0 -- not an asteroid (will add it to exclusion list)
21:18:30.94 +37:37:00.6 -- not an asteroid (will add it to exclusion list)
21:27:39.99 +41:28:15.9 -- not an asteroid (will add it to exclusion list)
21:15:31.87 +39:38:45.3 -- not an asteroid (will add it to exclusion list)
21:22:07.42 +37:28:58.6 -- not an asteroid (will add it to exclusion list)
21:13:30.27 +36:57:14.1 -- not an asteroid (will add it to exclusion list)
21:22:15.36 +39:25:45.8 -- not an asteroid (will add it to exclusion list)
21:12:30.88 +37:03:07.0 -- not an asteroid (will add it to exclusion list)
21:17:08.35 +38:25:40.4 -- not an asteroid (will add it to exclusion list)
21:15:47.29 +35:00:36.1 -- not an asteroid (will add it to exclusion list)
21:30:06.71 +42:42:51.2 -- not an asteroid (will add it to exclusion list)
21:09:14.84 +39:51:13.5 -- not an asteroid (will add it to exclusion list)
21:39:31.73 +40:39:06.9 -- not an asteroid (will add it to exclusion list)
21:21:45.46 +38:51:10.6 -- not an asteroid (will add it to exclusion list)
21:14:16.84 +37:13:45.6 -- not an asteroid (will add it to exclusion list)
21:52:14.88 +36:58:29.7 -- not an asteroid (will add it to exclusion list)
21:19:39.17 +33:52:22.4 -- not an asteroid (will add it to exclusion list)
21:14:59.61 +35:56:28.9 -- not an asteroid (will add it to exclusion list)
22:02:22.40 +41:34:46.0 -- not an asteroid (will add it to exclusion list)
21:15:38.33 +36:40:31.9 -- not an asteroid (will add it to exclusion list)
21:18:56.28 +38:50:10.9 -- not an asteroid (will add it to exclusion list)
21:29:27.20 +34:33:19.8 -- not an asteroid (will add it to exclusion list)
21:17:06.68 +41:12:00.4 -- not an asteroid (will add it to exclusion list)
21:35:28.32 +41:43:14.3 -- not an asteroid (will add it to exclusion list)
21:20:53.12 +35:23:53.9 -- not an asteroid (will add it to exclusion list)
21:28:05.33 +38:26:58.1 -- not an asteroid (will add it to exclusion list)
21:21:50.20 +36:52:22.5 -- not an asteroid (will add it to exclusion list)
21:15:26.44 +37:30:51.4 -- not an asteroid (will add it to exclusion list)
21:22:02.49 +35:07:47.2 -- not an asteroid (will add it to exclusion list)
21:22:02.31 +40:43:48.2 -- not an asteroid (will add it to exclusion list)
21:17:11.05 +36:26:19.7 -- not an asteroid (will add it to exclusion list)
21:24:04.31 +39:44:04.0 -- not an asteroid (will add it to exclusion list)
21:11:19.09 +37:30:42.3 -- not an asteroid (will add it to exclusion list)
21:09:57.15 +38:42:12.3 -- not an asteroid (will add it to exclusion list)
21:33:38.40 +34:07:28.0 -- not an asteroid (will add it to exclusion list)
21:24:44.61 +34:18:56.5 -- not an asteroid (will add it to exclusion list)
21:23:30.98 +34:11:51.6 -- not an asteroid (will add it to exclusion list)
21:15:36.01 +39:45:24.1 -- not an asteroid (will add it to exclusion list)
21:20:26.81 +34:06:13.7 -- not an asteroid (will add it to exclusion list)
21:09:54.44 +40:43:36.8 -- not an asteroid (will add it to exclusion list)
21:14:16.57 +40:58:14.5 -- not an asteroid (will add it to exclusion list)
22:06:26.75 +38:35:58.2 -- not an asteroid (will add it to exclusion list)
21:11:55.95 +39:55:31.5 -- not an asteroid (will add it to exclusion list)
21:27:06.47 +33:44:08.5 -- not an asteroid (will add it to exclusion list)
21:21:25.57 +36:56:48.2 -- not an asteroid (will add it to exclusion list)
21:24:48.14 +42:23:48.8 -- not an asteroid (will add it to exclusion list)
21:13:14.13 +42:38:33.7 -- not an asteroid (will add it to exclusion list)
21:16:57.10 +42:07:19.2 -- not an asteroid (will add it to exclusion list)
21:16:51.29 +37:38:57.4 -- not an asteroid (will add it to exclusion list)
21:08:48.24 +42:15:28.4 -- not an asteroid (will add it to exclusion list)
22:15:17.88 +37:28:35.3 -- not an asteroid (will add it to exclusion list)
21:26:55.09 +38:03:54.1 -- not an asteroid (will add it to exclusion list)
21:19:14.73 +35:22:02.5 -- not an asteroid (will add it to exclusion list)
21:32:06.88 +39:41:52.2 -- not an asteroid (will add it to exclusion list)
21:09:05.11 +42:36:25.8 -- not an asteroid (will add it to exclusion list)
21:13:06.79 +36:56:00.8 -- not an asteroid (will add it to exclusion list)
21:28:11.68 +40:25:03.1 -- not an asteroid (will add it to exclusion list)
21:12:33.74 +36:07:03.1 -- not an asteroid (will add it to exclusion list)
21:23:28.72 +41:52:46.5 -- not an asteroid (will add it to exclusion list)
21:14:16.35 +39:30:16.2 -- not an asteroid (will add it to exclusion list)
21:13:36.47 +40:33:16.4 -- not an asteroid (will add it to exclusion list)
21:28:24.99 +39:10:02.1 -- not an asteroid (will add it to exclusion list)
21:16:01.67 +41:46:07.3 -- not an asteroid (will add it to exclusion list)
21:26:05.34 +35:06:07.9 -- not an asteroid (will add it to exclusion list)
21:12:30.57 +39:48:04.7 -- not an asteroid (will add it to exclusion list)
21:12:21.74 +39:39:54.0 -- not an asteroid (will add it to exclusion list)
21:13:03.49 +36:09:05.9 -- not an asteroid (will add it to exclusion list)
21:22:43.62 +37:39:17.5 -- not an asteroid (will add it to exclusion list)
21:09:38.79 +38:16:13.8 -- not an asteroid (will add it to exclusion list)
21:26:10.16 +38:57:59.5 -- not an asteroid (will add it to exclusion list)
21:36:18.16 +40:03:04.6 -- not an asteroid (will add it to exclusion list)
21:15:44.18 +40:24:58.2 -- not an asteroid (will add it to exclusion list)
21:50:34.17 +37:11:04.4 -- not an asteroid (will add it to exclusion list)
21:31:39.14 +36:46:27.5 -- not an asteroid (will add it to exclusion list)
21:24:33.16 +35:18:35.4 -- not an asteroid (will add it to exclusion list)
21:12:13.58 +35:59:01.3 -- not an asteroid (will add it to exclusion list)
21:29:06.42 +42:10:44.9 -- not an asteroid (will add it to exclusion list)
21:21:51.44 +35:01:42.5 -- not an asteroid (will add it to exclusion list)
21:17:00.50 +40:40:07.8 -- not an asteroid (will add it to exclusion list)
21:43:03.17 +37:32:30.3 -- not an asteroid (will add it to exclusion list)
21:16:45.31 +37:40:26.8 -- not an asteroid (will add it to exclusion list)
21:20:36.52 +39:47:04.5 -- not an asteroid (will add it to exclusion list)
21:23:22.12 +39:56:38.4 -- not an asteroid (will add it to exclusion list)
21:17:14.63 +35:36:37.3 -- not an asteroid (will add it to exclusion list)
21:46:00.43 +37:21:18.7 -- not an asteroid (will add it to exclusion list)
21:25:09.83 +35:16:05.1 -- not an asteroid (will add it to exclusion list)
21:25:52.28 +34:14:43.9 -- not an asteroid (will add it to exclusion list)
21:28:04.36 +43:01:07.6 -- not an asteroid (will add it to exclusion list)
21:23:39.86 +36:34:06.7 -- not an asteroid (will add it to exclusion list)
21:13:26.53 +37:18:51.3 -- not an asteroid (will add it to exclusion list)
21:19:42.47 +42:04:26.7 -- not an asteroid (will add it to exclusion list)
21:48:47.70 +38:52:56.3 -- not an asteroid (will add it to exclusion list)
22:10:15.65 +41:33:59.3 -- not an asteroid (will add it to exclusion list)
22:20:33.29 +42:19:01.7 -- not an asteroid (will add it to exclusion list)
21:35:21.80 +41:16:18.5 -- not an asteroid (will add it to exclusion list)
21:20:38.41 +41:21:07.4 -- not an asteroid (will add it to exclusion list)
21:34:17.47 +36:20:30.1 -- not an asteroid (will add it to exclusion list)
21:19:00.61 +40:46:44.4 -- not an asteroid (will add it to exclusion list)
21:34:52.89 +37:58:12.8 -- not an asteroid (will add it to exclusion list)
21:17:18.89 +40:12:48.6 -- not an asteroid (will add it to exclusion list)
21:21:22.32 +39:19:41.6 -- not an asteroid (will add it to exclusion list)
21:23:41.27 +34:38:47.8 -- not an asteroid (will add it to exclusion list)
21:22:46.51 +41:12:15.2 -- not an asteroid (will add it to exclusion list)
21:14:55.67 +38:15:22.6 -- not an asteroid (will add it to exclusion list)
21:28:49.03 +41:29:04.0 -- not an asteroid (will add it to exclusion list)
22:07:43.00 +39:34:56.3 -- not an asteroid (will add it to exclusion list)
21:21:50.96 +37:08:26.3 -- not an asteroid (will add it to exclusion list)
21:21:17.06 +40:50:15.1 -- not an asteroid (will add it to exclusion list)
21:13:21.93 +42:19:57.4 -- not an asteroid (will add it to exclusion list)
21:13:50.26 +41:55:52.2 -- not an asteroid (will add it to exclusion list)
21:26:58.76 +38:06:04.9 -- not an asteroid (will add it to exclusion list)
21:43:55.49 +42:55:24.1 -- not an asteroid (will add it to exclusion list)
21:16:40.26 +38:16:21.7 -- not an asteroid (will add it to exclusion list)
21:31:28.06 +39:47:03.7 -- not an asteroid (will add it to exclusion list)
21:42:31.17 +35:51:15.0 -- not an asteroid (will add it to exclusion list)
21:43:09.61 +39:56:52.7 -- not an asteroid (will add it to exclusion list)
21:26:25.71 +40:35:04.0 -- not an asteroid (will add it to exclusion list)
21:16:04.57 +33:22:48.2 -- not an asteroid (will add it to exclusion list)
21:19:12.66 +42:09:19.6 -- not an asteroid (will add it to exclusion list)
21:20:48.36 +38:04:38.6 -- not an asteroid (will add it to exclusion list)
21:22:24.73 +38:01:28.6 -- not an asteroid (will add it to exclusion list)
21:13:13.48 +40:55:44.5 -- not an asteroid (will add it to exclusion list)
21:33:16.02 +41:46:48.1 -- not an asteroid (will add it to exclusion list)
21:16:51.47 +38:35:43.6 -- not an asteroid (will add it to exclusion list)
21:49:04.94 +37:22:34.1 -- not an asteroid (will add it to exclusion list)
21:28:43.64 +35:42:00.9 -- not an asteroid (will add it to exclusion list)
21:20:06.71 +36:34:21.2 -- not an asteroid (will add it to exclusion list)
21:15:57.26 +39:30:06.5 -- not an asteroid (will add it to exclusion list)
21:31:29.67 +33:55:39.5 -- not an asteroid (will add it to exclusion list)
21:10:23.61 +41:02:56.4 -- not an asteroid (will add it to exclusion list)
21:30:05.02 +40:57:00.0 -- not an asteroid (will add it to exclusion list)
21:24:21.77 +38:05:16.5 -- not an asteroid (will add it to exclusion list)
21:22:55.49 +41:49:49.9 -- not an asteroid (will add it to exclusion list)
21:50:40.28 +40:44:27.7 -- not an asteroid (will add it to exclusion list)
21:16:10.43 +38:43:55.8 -- not an asteroid (will add it to exclusion list)
21:12:05.84 +40:41:57.5 -- not an asteroid (will add it to exclusion list)
21:30:39.37 +38:36:13.0 -- not an asteroid (will add it to exclusion list)
21:16:40.15 +37:19:35.9 -- not an asteroid (will add it to exclusion list)
21:19:47.74 +36:39:52.8 -- not an asteroid (will add it to exclusion list)
21:19:40.11 +38:12:51.7 -- not an asteroid (will add it to exclusion list)
21:14:46.67 +40:23:26.2 -- not an asteroid (will add it to exclusion list)
21:18:11.75 +41:23:26.2 -- not an asteroid (will add it to exclusion list)
21:16:03.59 +37:34:29.4 -- not an asteroid (will add it to exclusion list)
21:11:48.52 +42:10:15.8 -- not an asteroid (will add it to exclusion list)
21:31:06.80 +39:46:47.2 -- not an asteroid (will add it to exclusion list)
21:18:56.70 +40:10:47.9 -- not an asteroid (will add it to exclusion list)
21:28:06.54 +36:36:22.2 -- not an asteroid (will add it to exclusion list)
21:15:24.90 +41:05:36.9 -- not an asteroid (will add it to exclusion list)
21:20:28.77 +35:50:51.5 -- not an asteroid (will add it to exclusion list)
21:11:22.27 +42:02:10.8 -- not an asteroid (will add it to exclusion list)
21:21:21.34 +38:00:17.5 -- not an asteroid (will add it to exclusion list)
21:24:31.55 +35:05:22.6 -- not an asteroid (will add it to exclusion list)
21:15:06.19 +37:57:17.8 -- not an asteroid (will add it to exclusion list)
22:22:57.31 +41:08:15.2 -- not an asteroid (will add it to exclusion list)
21:32:05.87 +40:41:03.1 -- not an asteroid (will add it to exclusion list)
21:17:05.36 +42:12:57.9 -- not an asteroid (will add it to exclusion list)
21:33:08.65 +41:21:51.9 -- not an asteroid (will add it to exclusion list)
21:12:36.49 +35:14:51.9 -- not an asteroid (will add it to exclusion list)
21:46:24.52 +41:13:01.9 -- not an asteroid (will add it to exclusion list)
21:28:44.93 +38:10:24.2 -- not an asteroid (will add it to exclusion list)
21:18:22.26 +37:39:43.5 -- not an asteroid (will add it to exclusion list)
21:19:08.62 +35:54:15.9 -- not an asteroid (will add it to exclusion list)
21:23:44.88 +38:52:26.7 -- not an asteroid (will add it to exclusion list)
21:37:50.58 +36:54:52.2 -- not an asteroid (will add it to exclusion list)
21:38:19.56 +39:47:35.3 -- not an asteroid (will add it to exclusion list)
22:21:26.07 +42:04:44.1 -- not an asteroid (will add it to exclusion list)
21:50:17.58 +42:04:56.8 -- not an asteroid (will add it to exclusion list)
21:23:42.42 +39:12:33.7 -- not an asteroid (will add it to exclusion list)
21:24:07.47 +35:25:05.5 -- not an asteroid (will add it to exclusion list)
21:19:21.90 +41:32:54.8 -- not an asteroid (will add it to exclusion list)
21:17:35.04 +42:45:34.5 -- not an asteroid (will add it to exclusion list)
21:34:40.18 +37:29:31.8 -- not an asteroid (will add it to exclusion list)
21:28:43.59 +35:11:00.7 -- not an asteroid (will add it to exclusion list)
21:43:18.74 +42:12:53.6 -- not an asteroid (will add it to exclusion list)
21:14:57.38 +39:59:29.7 -- not an asteroid (will add it to exclusion list)
21:32:16.35 +41:10:14.6 -- not an asteroid (will add it to exclusion list)
21:13:17.09 +40:02:29.8 -- not an asteroid (will add it to exclusion list)
21:37:42.98 +40:11:43.1 -- not an asteroid (will add it to exclusion list)
21:30:38.52 +36:36:07.3 -- not an asteroid (will add it to exclusion list)
21:12:32.95 +42:38:46.0 -- not an asteroid (will add it to exclusion list)
21:37:44.49 +42:39:12.3 -- not an asteroid (will add it to exclusion list)
21:46:20.85 +36:51:37.6 -- not an asteroid (will add it to exclusion list)
21:44:15.84 +42:45:31.0 -- not an asteroid (will add it to exclusion list)
21:26:53.39 +40:39:04.3 -- not an asteroid (will add it to exclusion list)
22:00:32.83 +39:39:03.1 -- not an asteroid (will add it to exclusion list)
21:20:55.89 +42:02:27.8 -- not an asteroid (will add it to exclusion list)
21:54:33.42 +35:50:15.0 -- not an asteroid (will add it to exclusion list)
21:55:49.52 +34:16:12.7 -- not an asteroid (will add it to exclusion list)
21:58:49.37 +40:28:42.2 -- not an asteroid (will add it to exclusion list)
21:25:47.96 +38:44:14.8 -- not an asteroid (will add it to exclusion list)
21:23:15.52 +40:06:52.5 -- not an asteroid (will add it to exclusion list)
21:21:11.28 +40:12:36.3 -- not an asteroid (will add it to exclusion list)
21:17:26.71 +36:06:08.9 -- not an asteroid (will add it to exclusion list)
22:11:18.63 +39:15:04.6 -- not an asteroid (will add it to exclusion list)
21:38:11.91 +37:42:54.7 -- not an asteroid (will add it to exclusion list)
21:38:48.53 +41:18:14.6 -- not an asteroid (will add it to exclusion list)
21:14:03.44 +35:50:46.0 -- not an asteroid (will add it to exclusion list)
21:41:20.41 +36:37:18.6 -- not an asteroid (will add it to exclusion list)
21:21:30.19 +39:05:33.9 -- not an asteroid (will add it to exclusion list)
21:37:02.07 +39:22:40.0 -- not an asteroid (will add it to exclusion list)
21:29:02.36 +41:37:46.7 -- not an asteroid (will add it to exclusion list)
21:31:05.87 +41:04:08.3 -- not an asteroid (will add it to exclusion list)
21:10:16.74 +40:21:12.6 -- not an asteroid (will add it to exclusion list)
21:53:37.45 +42:42:28.2 -- not an asteroid (will add it to exclusion list)
21:40:19.37 +35:38:56.5 -- not an asteroid (will add it to exclusion list)
21:52:16.26 +42:41:08.0 -- not an asteroid (will add it to exclusion list)
21:24:46.53 +35:05:09.9 -- not an asteroid (will add it to exclusion list)
21:21:59.18 +39:53:48.7 -- not an asteroid (will add it to exclusion list)
21:15:04.85 +39:19:08.4 -- not an asteroid (will add it to exclusion list)
21:13:00.22 +38:06:52.6 -- not an asteroid (will add it to exclusion list)
21:21:52.77 +34:43:08.5 -- not an asteroid (will add it to exclusion list)
21:41:27.40 +42:51:23.9 -- not an asteroid (will add it to exclusion list)
22:00:11.18 +39:37:38.7 -- not an asteroid (will add it to exclusion list)
21:36:26.19 +42:23:45.7 -- not an asteroid (will add it to exclusion list)
21:09:49.64 +38:21:37.4 -- not an asteroid (will add it to exclusion list)
21:14:30.73 +35:31:36.4 -- not an asteroid (will add it to exclusion list)
21:46:05.72 +42:50:03.3 -- not an asteroid (will add it to exclusion list)
21:28:40.79 +39:00:17.9 -- not an asteroid (will add it to exclusion list)
21:45:01.25 +42:15:60.0 -- not an asteroid (will add it to exclusion list)
21:33:09.21 +37:05:56.5 -- not an asteroid (will add it to exclusion list)
21:23:39.40 +38:42:01.8 -- not an asteroid (will add it to exclusion list)
21:35:31.04 +33:55:25.7 -- not an asteroid (will add it to exclusion list)
21:28:13.70 +33:56:53.8 -- not an asteroid (will add it to exclusion list)
21:32:31.54 +41:50:58.7 -- not an asteroid (will add it to exclusion list)
21:32:41.02 +38:29:40.1 -- not an asteroid (will add it to exclusion list)
21:39:50.83 +41:51:15.2 -- not an asteroid (will add it to exclusion list)
22:02:09.38 +41:51:02.7 -- not an asteroid (will add it to exclusion list)
21:55:25.46 +41:56:48.8 -- not an asteroid (will add it to exclusion list)
21:54:17.19 +36:52:11.4 -- not an asteroid (will add it to exclusion list)
21:26:28.37 +37:36:33.1 -- not an asteroid (will add it to exclusion list)
21:21:23.84 +33:48:25.1 -- not an asteroid (will add it to exclusion list)
21:31:17.20 +37:57:30.7 -- not an asteroid (will add it to exclusion list)
21:14:45.84 +36:18:04.1 -- not an asteroid (will add it to exclusion list)
21:24:27.69 +40:15:21.0 -- not an asteroid (will add it to exclusion list)
22:01:06.44 +42:14:35.8 -- not an asteroid (will add it to exclusion list)
21:16:12.44 +38:09:29.8 -- not an asteroid (will add it to exclusion list)
21:28:18.00 +34:05:00.0 -- not an asteroid (will add it to exclusion list)
21:56:20.29 +42:31:29.4 -- not an asteroid (will add it to exclusion list)
21:35:50.10 +39:03:54.1 -- not an asteroid (will add it to exclusion list)
21:33:40.41 +40:44:24.3 -- not an asteroid (will add it to exclusion list)
21:36:23.84 +37:34:30.9 -- not an asteroid (will add it to exclusion list)
21:20:02.87 +34:35:15.8 -- not an asteroid (will add it to exclusion list)
21:46:41.17 +40:55:18.6 -- not an asteroid (will add it to exclusion list)
21:30:24.45 +39:13:33.0 -- not an asteroid (will add it to exclusion list)
21:25:22.48 +36:07:15.0 -- not an asteroid (will add it to exclusion list)
21:49:31.96 +39:23:33.6 -- not an asteroid (will add it to exclusion list)
21:54:45.67 +38:18:18.0 -- not an asteroid (will add it to exclusion list)
21:24:23.57 +37:19:36.4 -- not an asteroid (will add it to exclusion list)
21:21:25.14 +36:00:11.8 -- not an asteroid (will add it to exclusion list)
22:09:31.96 +42:04:29.4 -- not an asteroid (will add it to exclusion list)
21:25:13.85 +34:03:17.5 -- not an asteroid (will add it to exclusion list)
21:32:24.91 +37:04:42.8 -- not an asteroid (will add it to exclusion list)
21:38:56.76 +37:31:12.5 -- not an asteroid (will add it to exclusion list)
21:40:15.33 +37:50:20.7 -- not an asteroid (will add it to exclusion list)
21:39:30.73 +37:21:41.9 -- not an asteroid (will add it to exclusion list)
21:52:59.99 +33:25:12.1 -- not an asteroid (will add it to exclusion list)
22:25:38.96 +39:59:37.6 -- not an asteroid (will add it to exclusion list)
22:23:25.16 +41:54:05.1 -- not an asteroid (will add it to exclusion list)
22:17:10.57 +41:19:17.1 -- not an asteroid (will add it to exclusion list)
21:57:38.14 +32:57:13.0 -- not an asteroid (will add it to exclusion list)
22:18:25.69 +41:03:50.0 -- not an asteroid (will add it to exclusion list)
22:23:57.60 +41:47:31.3 -- not an asteroid (will add it to exclusion list)
21:12:38.95 +33:09:36.0 -- not an asteroid (will add it to exclusion list)
22:24:39.80 +40:04:40.5 -- not an asteroid (will add it to exclusion list)
21:13:52.12 +34:18:26.4 -- not an asteroid (will add it to exclusion list)
22:27:04.57 +38:45:58.5 -- not an asteroid (will add it to exclusion list)
21:50:32.90 +33:17:12.9 -- not an asteroid (will add it to exclusion list)
21:28:06.78 +39:56:16.0 -- not an asteroid (will add it to exclusion list)
22:24:05.20 +39:13:30.0 -- not an asteroid (will add it to exclusion list)
22:20:30.72 +33:13:11.8 -- not an asteroid (will add it to exclusion list)
22:26:47.99 +39:55:16.8 -- not an asteroid (will add it to exclusion list)
22:27:15.22 +40:20:02.7 -- not an asteroid (will add it to exclusion list)
22:28:37.12 +40:06:52.2 -- not an asteroid (will add it to exclusion list)
22:27:39.56 +42:05:42.1 -- not an asteroid (will add it to exclusion list)
22:27:39.15 +41:18:21.0 -- not an asteroid (will add it to exclusion list)
22:22:07.59 +40:53:07.5 -- not an asteroid (will add it to exclusion list)
22:23:44.27 +32:54:14.5 -- not an asteroid (will add it to exclusion list)
22:12:21.99 +33:37:10.3 -- not an asteroid (will add it to exclusion list)
22:24:47.11 +40:38:54.7 -- not an asteroid (will add it to exclusion list)
22:21:42.03 +36:19:16.6 -- not an asteroid (will add it to exclusion list)
22:25:36.46 +40:51:52.1 -- not an asteroid (will add it to exclusion list)
22:25:10.79 +41:11:46.2 -- not an asteroid (will add it to exclusion list)
22:25:57.18 +40:25:48.2 -- not an asteroid (will add it to exclusion list)
22:23:00.35 +33:22:31.9 -- not an asteroid (will add it to exclusion list)
22:24:01.20 +39:08:02.8 -- not an asteroid (will add it to exclusion list)
22:26:30.26 +42:15:27.1 -- not an asteroid (will add it to exclusion list)
22:25:02.35 +38:38:36.5 -- not an asteroid (will add it to exclusion list)
22:27:43.44 +38:34:06.4 -- not an asteroid (will add it to exclusion list)
22:27:00.92 +41:35:40.0 -- not an asteroid (will add it to exclusion list)
22:22:34.15 +40:52:05.2 -- not an asteroid (will add it to exclusion list)
22:22:30.47 +41:47:35.7 -- not an asteroid (will add it to exclusion list)
22:27:09.21 +40:20:16.7 -- not an asteroid (will add it to exclusion list)
22:29:17.65 +41:28:02.2 -- not an asteroid (will add it to exclusion list)
22:25:38.23 +42:04:05.8 -- not an asteroid (will add it to exclusion list)
22:23:37.34 +38:47:39.1 -- not an asteroid (will add it to exclusion list)
22:27:53.50 +39:12:46.3 -- not an asteroid (will add it to exclusion list)
22:21:42.26 +40:38:49.2 -- not an asteroid (will add it to exclusion list)
22:21:12.77 +33:36:39.2 -- not an asteroid (will add it to exclusion list)
22:26:23.92 +39:12:21.1 -- not an asteroid (will add it to exclusion list)
22:23:32.73 +35:41:57.4 -- not an asteroid (will add it to exclusion list)
22:23:50.38 +40:10:59.7 -- not an asteroid (will add it to exclusion list)
22:21:09.27 +38:20:25.4 -- not an asteroid (will add it to exclusion list)
22:24:14.06 +41:20:03.0 -- not an asteroid (will add it to exclusion list)
22:26:22.35 +40:13:20.3 -- not an asteroid (will add it to exclusion list)
22:24:21.88 +37:53:04.8 -- not an asteroid (will add it to exclusion list)
22:27:32.23 +40:12:33.7 -- not an asteroid (will add it to exclusion list)
22:28:36.87 +41:59:19.8 -- not an asteroid (will add it to exclusion list)
22:24:47.79 +41:23:34.1 -- not an asteroid (will add it to exclusion list)
22:21:24.83 +40:44:14.1 -- not an asteroid (will add it to exclusion list)
22:24:29.96 +39:20:53.4 -- not an asteroid (will add it to exclusion list)
22:29:26.94 +40:50:02.5 -- not an asteroid (will add it to exclusion list)
22:28:16.73 +41:56:38.2 -- not an asteroid (will add it to exclusion list)
22:18:47.95 +40:40:39.3 -- not an asteroid (will add it to exclusion list)
22:19:47.33 +42:24:09.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:08:48.24 +42:15:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:04.49 +40:48:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:05.11 +42:36:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:14.84 +39:51:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:31.20 +40:48:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:38.79 +38:16:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:49.64 +38:21:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:53.82 +42:17:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:54.44 +40:43:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:56.53 +42:31:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:57.15 +38:42:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:58.24 +38:52:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:16.74 +40:21:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:23.61 +41:02:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:24.23 +38:26:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:29.46 +36:14:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:46.12 +35:46:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:56.05 +35:44:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:00.67 +40:05:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:10.88 +35:31:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:16.17 +36:08:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:19.09 +37:30:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:20.88 +39:12:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:22.27 +42:02:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:33.88 +36:22:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:38.29 +37:30:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:38.47 +38:20:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:46.96 +36:20:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:48.52 +42:10:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:50.84 +40:34:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:51.11 +35:37:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:55.95 +39:55:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:57.97 +36:45:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:58.18 +34:50:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:04.94 +42:34:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:05.84 +40:41:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:13.58 +35:59:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:13.97 +35:19:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:21.74 +39:39:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:24.20 +40:10:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:24.72 +33:36:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:30.57 +39:48:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:30.88 +37:03:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:32.95 +42:38:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:33.74 +36:07:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:36.49 +35:14:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:38.13 +39:31:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:38.95 +33:09:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:39.54 +38:09:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:41.04 +33:09:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:44.35 +36:07:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:46.98 +42:24:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:49.51 +41:23:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:50.84 +36:08:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:59.88 +36:04:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:00.22 +38:06:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:03.05 +33:40:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:03.49 +36:09:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:06.79 +36:56:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:09.70 +38:07:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:13.48 +40:55:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:14.13 +42:38:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:16.12 +33:44:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:16.20 +41:07:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:17.09 +40:02:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:21.93 +42:19:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:26.53 +37:18:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:30.27 +36:57:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:36.47 +40:33:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:50.26 +41:55:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:52.12 +34:18:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:58.07 +36:59:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:58.21 +36:11:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:03.36 +34:52:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:03.44 +35:50:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:07.41 +39:48:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:10.55 +37:06:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:10.79 +37:29:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:14.01 +36:03:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:16.35 +39:30:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:16.57 +40:58:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:16.84 +37:13:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:26.33 +37:57:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:30.73 +35:31:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:34.90 +37:36:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:38.40 +37:33:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:40.71 +37:16:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:40.80 +39:49:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:41.33 +34:18:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:41.88 +36:07:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:44.84 +38:12:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:45.84 +36:18:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:46.67 +40:23:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:48.66 +37:08:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:51.36 +38:32:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:54.60 +34:58:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:55.67 +38:15:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:57.38 +39:59:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:58.71 +40:12:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:59.46 +34:09:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:59.61 +35:56:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:01.14 +37:38:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:04.85 +39:19:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:06.19 +37:57:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:07.43 +38:34:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:17.47 +38:56:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:24.90 +41:05:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:25.79 +36:10:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:26.44 +37:30:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:31.73 +38:37:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:31.87 +39:38:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:36.01 +39:45:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:36.32 +36:55:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:38.33 +36:40:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:42.98 +33:53:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:44.18 +40:24:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:45.32 +36:35:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:47.29 +35:00:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:47.41 +37:50:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:57.26 +39:30:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:01.67 +41:46:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:03.59 +37:34:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:04.57 +33:22:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:05.12 +35:26:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:06.05 +38:52:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:10.43 +38:43:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:12.44 +38:09:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:22.33 +37:47:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:29.78 +36:27:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:35.26 +37:06:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:40.15 +37:19:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:40.26 +38:16:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:43.12 +41:35:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:44.97 +34:40:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:45.31 +37:40:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:51.29 +37:38:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:51.47 +38:35:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:52.19 +40:29:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:57.10 +42:07:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:57.74 +37:32:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:00.50 +40:40:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:03.32 +37:35:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:05.36 +42:12:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:06.42 +35:11:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:06.68 +41:12:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:08.35 +38:25:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:11.05 +36:26:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:13.96 +41:04:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:14.63 +35:36:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:15.26 +35:51:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:15.27 +41:40:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:15.71 +34:09:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:18.89 +40:12:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:19.92 +34:34:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:20.41 +36:43:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:26.71 +36:06:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:35.04 +42:45:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:44.76 +38:40:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:50.23 +39:58:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:51.46 +37:12:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:56.57 +39:27:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:59.54 +42:35:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:02.81 +41:31:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:11.75 +41:23:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:22.26 +37:39:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:25.07 +38:04:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:26.61 +34:17:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:30.94 +37:37:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:36.52 +38:08:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:37.33 +33:54:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:43.48 +37:57:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:44.62 +36:41:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:50.95 +34:56:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:55.54 +41:30:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:56.28 +38:50:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:56.70 +40:10:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:00.61 +40:46:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:04.73 +38:33:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:08.62 +35:54:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:12.66 +42:09:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:14.73 +35:22:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:18.15 +42:26:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:19.25 +39:41:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:21.90 +41:32:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:25.52 +34:12:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:28.79 +39:57:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:37.43 +35:07:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:39.17 +33:52:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:40.11 +38:12:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:42.35 +38:45:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:42.47 +42:04:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:47.74 +36:39:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:52.54 +38:04:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:02.87 +34:35:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:06.58 +39:26:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:06.71 +36:34:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:10.14 +33:10:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:25.11 +37:31:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:26.81 +34:06:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:28.77 +35:50:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:36.52 +39:47:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:37.24 +41:57:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:38.41 +41:21:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:39.63 +40:14:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:48.36 +38:04:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:50.00 +33:44:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:52.17 +38:17:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:53.12 +35:23:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:55.89 +42:02:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:04.51 +40:28:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:06.53 +36:01:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:11.28 +40:12:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:12.52 +36:20:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:17.06 +40:50:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:21.34 +38:00:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:22.32 +39:19:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:23.82 +41:56:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:23.84 +33:48:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:25.14 +36:00:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:25.57 +36:56:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:29.43 +39:04:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:30.19 +39:05:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:41.70 +36:14:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:45.46 +38:51:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:47.77 +35:29:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:50.20 +36:52:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:50.96 +37:08:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:51.44 +35:01:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:52.77 +34:43:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:53.02 +41:39:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:59.18 +39:53:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:02.31 +40:43:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:02.49 +35:07:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:07.42 +37:28:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:15.36 +39:25:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:24.73 +38:01:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:28.29 +40:43:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:36.12 +35:35:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:43.62 +37:39:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:46.51 +41:12:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:48.69 +36:59:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:55.49 +41:49:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:15.52 +40:06:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:22.12 +39:56:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:28.72 +41:52:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:30.98 +34:11:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:35.11 +38:21:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:39.40 +38:42:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:39.86 +36:34:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:41.27 +34:38:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:42.42 +39:12:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:44.88 +38:52:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:04.31 +39:44:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:07.47 +35:25:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:11.07 +37:39:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:21.77 +38:05:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:23.57 +37:19:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:27.69 +40:15:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:31.55 +35:05:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:33.16 +35:18:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:39.66 +36:58:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:42.39 +38:26:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:44.61 +34:18:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:46.53 +35:05:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:48.14 +42:23:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:53.95 +33:31:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:56.62 +36:58:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:57.22 +42:40:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:03.54 +33:29:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:09.83 +35:16:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:10.17 +35:57:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:13.85 +34:03:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:22.48 +36:07:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:27.48 +37:40:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:47.96 +38:44:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:52.28 +34:14:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:56.52 +38:11:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:05.34 +35:06:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:10.16 +38:57:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:11.09 +42:43:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:25.16 +35:51:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:25.71 +40:35:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:27.74 +35:10:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:28.37 +37:36:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:38.61 +39:47:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:50.82 +42:27:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.16 +37:31:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.39 +40:39:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:55.09 +38:03:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:58.76 +38:06:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:06.47 +33:44:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:09.80 +36:53:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:12.32 +39:44:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:27.41 +38:09:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:28.52 +35:23:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:31.59 +35:50:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:39.99 +41:28:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:59.74 +37:32:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:00.13 +36:42:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:04.36 +43:01:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:05.33 +38:26:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.54 +36:36:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.78 +39:56:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:11.68 +40:25:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:13.70 +33:56:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:14.41 +42:51:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:18.00 +34:05:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:24.99 +39:10:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:37.89 +35:33:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:40.79 +39:00:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:41.55 +42:35:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.59 +35:11:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.64 +35:42:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:44.93 +38:10:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:49.03 +41:29:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.59 +35:14:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:02.36 +41:37:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:04.95 +40:27:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:06.42 +42:10:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:08.03 +42:01:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:27.20 +34:33:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:32.10 +33:48:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:38.32 +39:05:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:05.02 +40:57:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:06.71 +42:42:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:24.45 +39:13:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:37.79 +42:45:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:38.52 +36:36:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:39.37 +38:36:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:49.11 +38:57:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:05.87 +41:04:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:06.80 +39:46:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:14.91 +38:46:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:17.20 +37:57:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:28.06 +39:47:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:29.67 +33:55:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:39.14 +36:46:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:05.87 +40:41:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:06.88 +39:41:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:16.35 +41:10:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:24.91 +37:04:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:26.27 +37:28:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:28.08 +38:05:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:31.54 +41:50:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:41.02 +38:29:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:48.30 +39:29:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:08.65 +41:21:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:09.21 +37:05:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:16.02 +41:46:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:38.40 +34:07:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:40.41 +40:44:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:53.13 +33:18:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:11.25 +40:41:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:17.47 +36:20:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:40.18 +37:29:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:52.89 +37:58:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:59.13 +39:59:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:21.80 +41:16:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:23.88 +36:47:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:24.40 +36:45:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:28.32 +41:43:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:31.04 +33:55:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:50.10 +39:03:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:50.35 +40:48:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:15.14 +40:02:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:18.16 +40:03:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:23.84 +37:34:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:26.19 +42:23:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:48.43 +38:51:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:54.29 +40:36:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:02.07 +39:22:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:34.51 +32:59:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:35.64 +40:12:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:42.98 +40:11:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:44.49 +42:39:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:50.58 +36:54:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:54.69 +33:00:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:11.91 +37:42:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:19.56 +39:47:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:48.53 +41:18:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:56.76 +37:31:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:02.90 +40:22:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:30.73 +37:21:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:31.73 +40:39:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:47.29 +42:43:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:50.83 +41:51:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:15.33 +37:50:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:19.25 +38:45:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:19.37 +35:38:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:23.65 +39:00:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:35.21 +39:13:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:47.73 +38:06:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:18.31 +41:17:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:20.41 +36:37:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:27.40 +42:51:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:50.86 +35:55:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:06.01 +36:50:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:23.05 +40:36:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:23.52 +41:49:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:31.17 +35:51:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:46.31 +37:59:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:03.17 +37:32:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:09.61 +39:56:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:18.74 +42:12:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:35.18 +37:22:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:36.58 +42:31:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:42.41 +42:34:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:55.49 +42:55:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:15.84 +42:45:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:49.72 +36:56:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:01.25 +42:15:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:30.06 +40:39:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:00.43 +37:21:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:05.72 +42:50:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:08.61 +35:33:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:20.85 +36:51:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:24.52 +41:13:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:34.06 +35:50:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:41.17 +40:55:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:53.87 +39:15:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:46.98 +40:08:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.70 +38:52:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:04.94 +37:22:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:31.96 +39:23:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:54.44 +34:54:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:11.43 +35:33:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:17.58 +42:04:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:32.90 +33:17:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:34.17 +37:11:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:40.28 +40:44:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:49.89 +33:01:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:38.10 +43:02:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:14.88 +36:58:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:16.26 +42:41:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:59.99 +33:25:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:17.43 +42:34:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:19.50 +34:36:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:37.45 +42:42:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:17.19 +36:52:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:33.42 +35:50:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:45.67 +38:18:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:25.46 +41:56:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:49.52 +34:16:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.37 +37:10:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:08.18 +40:50:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:20.29 +42:31:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:29.02 +36:52:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:32.95 +38:17:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:34.36 +37:00:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:49.58 +42:13:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:38.14 +32:57:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:39.23 +41:47:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:59.24 +41:37:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:13.38 +38:26:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:49.37 +40:28:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:30.86 +42:08:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:59.93 +38:42:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:11.18 +39:37:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:15.47 +42:40:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:32.83 +39:39:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:03.93 +41:04:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:06.44 +42:14:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:07.92 +39:15:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.36 +40:55:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:26.89 +38:07:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:57.33 +35:42:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:04.51 +37:45:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:09.38 +41:51:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:13.82 +41:47:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.40 +41:34:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:27.71 +42:04:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:36.81 +38:54:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:01.96 +41:27:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:11.01 +42:22:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:11.22 +41:31:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:53.83 +33:29:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:26.75 +38:35:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:46.45 +39:39:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:54.81 +41:38:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:43.00 +39:34:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:43.26 +37:37:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:49.45 +33:25:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:04.65 +35:52:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:32.91 +35:58:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:11.24 +36:46:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:13.49 +39:15:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:21.19 +33:46:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:23.69 +40:29:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:31.96 +42:04:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:56.43 +39:05:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:15.65 +41:33:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:18.63 +39:15:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:04.42 +37:38:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:21.99 +33:37:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:22.91 +41:42:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:26.42 +40:34:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:03.48 +38:28:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:08.46 +40:02:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:09.47 +38:28:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:17.49 +39:47:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:17.88 +37:28:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:54.18 +37:58:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:10.57 +41:19:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:24.47 +38:35:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:25.04 +42:04:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:45.88 +39:00:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:25.69 +41:03:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:47.95 +40:40:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:20.15 +40:03:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:47.33 +42:24:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:24.64 +41:35:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:30.72 +33:13:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:30.94 +33:33:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:33.29 +42:19:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:44.67 +42:23:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:09.27 +38:20:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:12.77 +33:36:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:21.34 +41:17:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:24.16 +41:17:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:24.83 +40:44:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:26.07 +42:04:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:42.03 +36:19:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:42.26 +40:38:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:51.89 +38:05:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:07.59 +40:53:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:30.47 +41:47:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:34.15 +40:52:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:57.31 +41:08:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:00.35 +33:22:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:06.22 +41:02:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:25.16 +41:54:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:32.73 +35:41:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:37.34 +38:47:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:41.87 +34:37:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:44.27 +32:54:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:50.38 +40:10:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:57.60 +41:47:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:00.62 +40:01:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:01.20 +39:08:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:04.86 +41:24:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:05.20 +39:13:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:14.06 +41:20:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:21.88 +37:53:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:29.96 +39:20:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:31.98 +41:49:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:39.80 +40:04:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:43.50 +41:45:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:47.11 +40:38:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:47.79 +41:23:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:02.35 +38:38:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:10.79 +41:11:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:36.46 +40:51:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:38.23 +42:04:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:38.96 +39:59:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:57.18 +40:25:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:17.45 +40:38:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:22.35 +40:13:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:23.92 +39:12:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:27.62 +39:49:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:30.26 +42:15:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:35.03 +36:53:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:44.89 +40:34:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:47.99 +39:55:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:26:53.22 +41:24:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:00.92 +41:35:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:04.57 +38:45:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:09.21 +40:20:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:14.92 +42:09:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:15.22 +40:20:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:32.23 +40:12:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:39.15 +41:18:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:39.56 +42:05:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:43.44 +38:34:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:53.50 +39:12:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:59.83 +41:57:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:16.73 +41:56:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:36.87 +41:59:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:37.12 +40:06:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:39.45 +41:36:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:45.72 +41:44:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:17.65 +41:28:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:26.94 +40:50:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:53.35 +41:26:00.2 -- 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)
21:08:48.24 +42:15:28.4 -- not a known variable star
21:09:04.49 +40:48:05.6 -- not a known variable star
21:09:05.11 +42:36:25.8 -- not a known variable star
21:09:14.84 +39:51:13.5 -- a known variable star
21:09:31.20 +40:48:31.9 -- a known variable star
21:09:38.79 +38:16:13.8 -- not a known variable star
21:09:49.64 +38:21:37.4 -- not a known variable star
21:09:53.82 +42:17:25.4 -- a known variable star
21:09:54.44 +40:43:36.8 -- not a known variable star
21:09:56.53 +42:31:27.0 -- a known variable star
21:09:57.15 +38:42:12.3 -- not a known variable star
21:09:58.24 +38:52:34.6 -- not a known variable star
21:10:16.74 +40:21:12.6 -- not a known variable star
21:10:23.61 +41:02:56.4 -- not a known variable star
21:10:24.23 +38:26:35.0 -- not a known variable star
21:10:29.46 +36:14:17.0 -- not a known variable star
21:10:46.12 +35:46:39.9 -- a known variable star
21:10:56.05 +35:44:07.0 -- not a known variable star
21:11:00.67 +40:05:05.5 -- not a known variable star
21:11:10.88 +35:31:16.4 -- not a known variable star
21:11:16.17 +36:08:41.0 -- not a known variable star
21:11:19.09 +37:30:42.3 -- not a known variable star
21:11:20.88 +39:12:54.3 -- not a known variable star
21:11:22.27 +42:02:10.8 -- not a known variable star
21:11:33.88 +36:22:57.6 -- not a known variable star
21:11:38.29 +37:30:37.3 -- not a known variable star
21:11:38.47 +38:20:47.4 -- not a known variable star
21:11:46.96 +36:20:55.9 -- a known variable star
21:11:48.52 +42:10:15.8 -- not a known variable star
21:11:50.84 +40:34:54.6 -- not a known variable star
21:11:51.11 +35:37:58.7 -- not a known variable star
21:11:55.95 +39:55:31.5 -- not a known variable star
21:11:57.97 +36:45:24.9 -- not a known variable star
21:11:58.18 +34:50:23.8 -- not a known variable star
21:12:04.94 +42:34:05.0 -- not a known variable star
21:12:05.84 +40:41:57.5 -- not a known variable star
21:12:13.58 +35:59:01.3 -- not a known variable star
21:12:13.97 +35:19:19.8 -- a known variable star
21:12:21.74 +39:39:54.0 -- not a known variable star
21:12:24.20 +40:10:31.1 -- not a known variable star
21:12:24.72 +33:36:18.5 -- a known variable star
21:12:30.57 +39:48:04.7 -- a known variable star
21:12:30.88 +37:03:07.0 -- not a known variable star
21:12:32.95 +42:38:46.0 -- not a known variable star
21:12:33.74 +36:07:03.1 -- not a known variable star
21:12:36.49 +35:14:51.9 -- not a known variable star
21:12:38.13 +39:31:59.6 -- not a known variable star
21:12:38.95 +33:09:36.0 -- not a known variable star
21:12:39.54 +38:09:44.1 -- not a known variable star
21:12:41.04 +33:09:48.9 -- not a known variable star
21:12:44.35 +36:07:58.7 -- not a known variable star
21:12:46.98 +42:24:03.8 -- not a known variable star
21:12:49.51 +41:23:27.4 -- a known variable star
21:12:50.84 +36:08:07.8 -- not a known variable star
21:12:59.88 +36:04:17.9 -- not a known variable star
21:13:00.22 +38:06:52.6 -- not a known variable star
21:13:03.05 +33:40:45.7 -- not a known variable star
21:13:03.49 +36:09:05.9 -- not a known variable star
21:13:06.79 +36:56:00.8 -- not a known variable star
21:13:09.70 +38:07:24.2 -- not a known variable star
21:13:13.48 +40:55:44.5 -- not a known variable star
21:13:14.13 +42:38:33.7 -- not a known variable star
21:13:16.12 +33:44:29.7 -- not a known variable star
21:13:16.20 +41:07:40.5 -- not a known variable star
21:13:17.09 +40:02:29.8 -- not a known variable star
21:13:21.93 +42:19:57.4 -- not a known variable star
21:13:26.53 +37:18:51.3 -- not a known variable star
21:13:30.27 +36:57:14.1 -- not a known variable star
21:13:36.47 +40:33:16.4 -- not a known variable star
21:13:50.26 +41:55:52.2 -- not a known variable star
21:13:52.12 +34:18:26.4 -- not a known variable star
21:13:58.07 +36:59:38.7 -- not a known variable star
21:13:58.21 +36:11:59.5 -- not a known variable star
21:14:03.36 +34:52:46.8 -- not a known variable star
21:14:03.44 +35:50:46.0 -- not a known variable star
21:14:07.41 +39:48:24.2 -- not a known variable star
21:14:10.55 +37:06:09.0 -- not a known variable star
21:14:10.79 +37:29:35.0 -- not a known variable star
21:14:14.01 +36:03:26.7 -- not a known variable star
21:14:16.35 +39:30:16.2 -- not a known variable star
21:14:16.57 +40:58:14.5 -- not a known variable star
21:14:16.84 +37:13:45.6 -- not a known variable star
21:14:26.33 +37:57:13.1 -- not a known variable star
21:14:30.73 +35:31:36.4 -- not a known variable star
21:14:34.90 +37:36:52.5 -- not a known variable star
21:14:38.40 +37:33:48.6 -- not a known variable star
21:14:40.71 +37:16:07.6 -- not a known variable star
21:14:40.80 +39:49:56.5 -- not a known variable star
21:14:41.33 +34:18:39.8 -- a known variable star
21:14:41.88 +36:07:14.6 -- not a known variable star
21:14:44.84 +38:12:03.0 -- not a known variable star
21:14:45.84 +36:18:04.1 -- not a known variable star
21:14:46.67 +40:23:26.2 -- not a known variable star
21:14:48.66 +37:08:03.6 -- not a known variable star
21:14:51.36 +38:32:19.8 -- not a known variable star
21:14:54.60 +34:58:50.3 -- not a known variable star
21:14:55.67 +38:15:22.6 -- not a known variable star
21:14:57.38 +39:59:29.7 -- not a known variable star
21:14:58.71 +40:12:43.0 -- not a known variable star
21:14:59.46 +34:09:50.9 -- not a known variable star
21:14:59.61 +35:56:28.9 -- not a known variable star
21:15:01.14 +37:38:00.8 -- not a known variable star
21:15:04.85 +39:19:08.4 -- not a known variable star
21:15:06.19 +37:57:17.8 -- not a known variable star
21:15:07.43 +38:34:26.4 -- not a known variable star
21:15:17.47 +38:56:43.3 -- not a known variable star
21:15:24.90 +41:05:36.9 -- not a known variable star
21:15:25.79 +36:10:50.5 -- not a known variable star
21:15:26.44 +37:30:51.4 -- not a known variable star
21:15:31.73 +38:37:42.4 -- not a known variable star
21:15:31.87 +39:38:45.3 -- not a known variable star
21:15:36.01 +39:45:24.1 -- not a known variable star
21:15:36.32 +36:55:35.8 -- not a known variable star
21:15:38.33 +36:40:31.9 -- not a known variable star
21:15:42.98 +33:53:35.1 -- not a known variable star
21:15:44.18 +40:24:58.2 -- not a known variable star
21:15:45.32 +36:35:09.8 -- not a known variable star
21:15:47.29 +35:00:36.1 -- a known variable star
21:15:47.41 +37:50:42.3 -- a known variable star
21:15:57.26 +39:30:06.5 -- not a known variable star
21:16:01.67 +41:46:07.3 -- not a known variable star
21:16:03.59 +37:34:29.4 -- not a known variable star
21:16:04.57 +33:22:48.2 -- not a known variable star
21:16:05.12 +35:26:56.5 -- not a known variable star
21:16:06.05 +38:52:02.3 -- not a known variable star
21:16:10.43 +38:43:55.8 -- not a known variable star
21:16:12.44 +38:09:29.8 -- not a known variable star
21:16:22.33 +37:47:56.0 -- not a known variable star
21:16:29.78 +36:27:23.2 -- not a known variable star
21:16:35.26 +37:06:18.1 -- not a known variable star
21:16:40.15 +37:19:35.9 -- not a known variable star
21:16:40.26 +38:16:21.7 -- not a known variable star
21:16:43.12 +41:35:51.4 -- a known variable star
21:16:44.97 +34:40:58.5 -- not a known variable star
21:16:45.31 +37:40:26.8 -- not a known variable star
21:16:51.29 +37:38:57.4 -- not a known variable star
21:16:51.47 +38:35:43.6 -- a known variable star
21:16:52.19 +40:29:56.3 -- not a known variable star
21:16:57.10 +42:07:19.2 -- not a known variable star
21:16:57.74 +37:32:50.0 -- not a known variable star
21:17:00.50 +40:40:07.8 -- not a known variable star
21:17:03.32 +37:35:40.5 -- a known variable star
21:17:05.36 +42:12:57.9 -- a known variable star
21:17:06.42 +35:11:34.0 -- not a known variable star
21:17:06.68 +41:12:00.4 -- not a known variable star
21:17:08.35 +38:25:40.4 -- not a known variable star
21:17:11.05 +36:26:19.7 -- not a known variable star
21:17:13.96 +41:04:32.0 -- not a known variable star
21:17:14.63 +35:36:37.3 -- not a known variable star
21:17:15.26 +35:51:06.5 -- not a known variable star
21:17:15.27 +41:40:01.8 -- not a known variable star
21:17:15.71 +34:09:14.6 -- a known variable star
21:17:18.89 +40:12:48.6 -- not a known variable star
21:17:19.92 +34:34:11.1 -- not a known variable star
21:17:20.41 +36:43:54.8 -- not a known variable star
21:17:26.71 +36:06:08.9 -- not a known variable star
21:17:35.04 +42:45:34.5 -- not a known variable star
21:17:44.76 +38:40:34.1 -- not a known variable star
21:17:50.23 +39:58:39.7 -- not a known variable star
21:17:51.46 +37:12:27.1 -- a known variable star
21:17:56.57 +39:27:24.9 -- not a known variable star
21:17:59.54 +42:35:34.7 -- not a known variable star
21:18:02.81 +41:31:39.7 -- not a known variable star
21:18:11.75 +41:23:26.2 -- not a known variable star
21:18:22.26 +37:39:43.5 -- not a known variable star
21:18:25.07 +38:04:45.1 -- not a known variable star
21:18:26.61 +34:17:33.4 -- a known variable star
21:18:30.94 +37:37:00.6 -- not a known variable star
21:18:36.52 +38:08:19.0 -- not a known variable star
21:18:37.33 +33:54:03.0 -- not a known variable star
21:18:43.48 +37:57:52.4 -- not a known variable star
21:18:44.62 +36:41:41.9 -- not a known variable star
21:18:50.95 +34:56:39.7 -- not a known variable star
21:18:55.54 +41:30:47.1 -- not a known variable star
21:18:56.28 +38:50:10.9 -- not a known variable star
21:18:56.70 +40:10:47.9 -- not a known variable star
21:19:00.61 +40:46:44.4 -- a known variable star
21:19:04.73 +38:33:58.2 -- not a known variable star
21:19:08.62 +35:54:15.9 -- not a known variable star
21:19:12.66 +42:09:19.6 -- not a known variable star
21:19:14.73 +35:22:02.5 -- not a known variable star
21:19:18.15 +42:26:13.0 -- not a known variable star
21:19:19.25 +39:41:30.2 -- not a known variable star
21:19:21.90 +41:32:54.8 -- not a known variable star
21:19:25.52 +34:12:50.4 -- not a known variable star
21:19:28.79 +39:57:40.4 -- not a known variable star
21:19:37.43 +35:07:20.3 -- not a known variable star
21:19:39.17 +33:52:22.4 -- not a known variable star
21:19:40.11 +38:12:51.7 -- not a known variable star
21:19:42.35 +38:45:32.1 -- not a known variable star
21:19:42.47 +42:04:26.7 -- not a known variable star
21:19:47.74 +36:39:52.8 -- not a known variable star
21:19:52.54 +38:04:01.1 -- not a known variable star
21:20:02.87 +34:35:15.8 -- not a known variable star
21:20:06.58 +39:26:52.7 -- not a known variable star
21:20:06.71 +36:34:21.2 -- not a known variable star
21:20:10.14 +33:10:26.1 -- not a known variable star
21:20:25.11 +37:31:57.3 -- not a known variable star
21:20:26.81 +34:06:13.7 -- not a known variable star
21:20:28.77 +35:50:51.5 -- not a known variable star
21:20:36.52 +39:47:04.5 -- a known variable star
21:20:37.24 +41:57:32.3 -- a known variable star
21:20:38.41 +41:21:07.4 -- not a known variable star
21:20:39.63 +40:14:13.6 -- a known variable star
21:20:48.36 +38:04:38.6 -- not a known variable star
21:20:50.00 +33:44:17.2 -- not a known variable star
21:20:52.17 +38:17:39.5 -- not a known variable star
21:20:53.12 +35:23:53.9 -- not a known variable star
21:20:55.89 +42:02:27.8 -- not a known variable star
21:21:04.51 +40:28:37.5 -- not a known variable star
21:21:06.53 +36:01:47.5 -- not a known variable star
21:21:11.28 +40:12:36.3 -- not a known variable star
21:21:12.52 +36:20:37.3 -- not a known variable star
21:21:17.06 +40:50:15.1 -- a known variable star
21:21:21.34 +38:00:17.5 -- not a known variable star
21:21:22.32 +39:19:41.6 -- not a known variable star
21:21:23.82 +41:56:52.4 -- not a known variable star
21:21:23.84 +33:48:25.1 -- not a known variable star
21:21:25.14 +36:00:11.8 -- not a known variable star
21:21:25.57 +36:56:48.2 -- not a known variable star
21:21:29.43 +39:04:36.5 -- a known variable star
21:21:30.19 +39:05:33.9 -- not a known variable star
21:21:41.70 +36:14:58.9 -- not a known variable star
21:21:45.46 +38:51:10.6 -- not a known variable star
21:21:47.77 +35:29:50.0 -- not a known variable star
21:21:50.20 +36:52:22.5 -- not a known variable star
21:21:50.96 +37:08:26.3 -- not a known variable star
21:21:51.44 +35:01:42.5 -- a known variable star
21:21:52.77 +34:43:08.5 -- not a known variable star
21:21:53.02 +41:39:20.3 -- not a known variable star
21:21:59.18 +39:53:48.7 -- not a known variable star
21:22:02.31 +40:43:48.2 -- not a known variable star
21:22:02.49 +35:07:47.2 -- not a known variable star
21:22:07.42 +37:28:58.6 -- not a known variable star
21:22:15.36 +39:25:45.8 -- not a known variable star
21:22:24.73 +38:01:28.6 -- not a known variable star
21:22:28.29 +40:43:48.8 -- not a known variable star
21:22:36.12 +35:35:48.8 -- not a known variable star
21:22:43.62 +37:39:17.5 -- not a known variable star
21:22:46.51 +41:12:15.2 -- not a known variable star
21:22:48.69 +36:59:03.9 -- a known variable star
21:22:55.49 +41:49:49.9 -- not a known variable star
21:23:15.52 +40:06:52.5 -- not a known variable star
21:23:22.12 +39:56:38.4 -- not a known variable star
21:23:28.72 +41:52:46.5 -- not a known variable star
21:23:30.98 +34:11:51.6 -- not a known variable star
21:23:35.11 +38:21:41.0 -- not a known variable star
21:23:39.40 +38:42:01.8 -- not a known variable star
21:23:39.86 +36:34:06.7 -- a known variable star
21:23:41.27 +34:38:47.8 -- not a known variable star
21:23:42.42 +39:12:33.7 -- a known variable star
21:23:44.88 +38:52:26.7 -- not a known variable star
21:24:04.31 +39:44:04.0 -- not a known variable star
21:24:07.47 +35:25:05.5 -- a known variable star
21:24:11.07 +37:39:45.7 -- not a known variable star
21:24:21.77 +38:05:16.5 -- not a known variable star
21:24:23.57 +37:19:36.4 -- not a known variable star
21:24:27.69 +40:15:21.0 -- not a known variable star
21:24:31.55 +35:05:22.6 -- not a known variable star
21:24:33.16 +35:18:35.4 -- not a known variable star
21:24:39.66 +36:58:46.5 -- a known variable star
21:24:42.39 +38:26:36.8 -- a known variable star
21:24:44.61 +34:18:56.5 -- not a known variable star
21:24:46.53 +35:05:09.9 -- not a known variable star
21:24:48.14 +42:23:48.8 -- a known variable star
21:24:53.95 +33:31:57.4 -- a known variable star
21:24:56.62 +36:58:07.4 -- a known variable star
21:24:57.22 +42:40:16.6 -- a known variable star
21:25:03.54 +33:29:46.4 -- not a known variable star
21:25:09.83 +35:16:05.1 -- not a known variable star
21:25:10.17 +35:57:12.1 -- a known variable star
21:25:13.85 +34:03:17.5 -- not a known variable star
21:25:22.48 +36:07:15.0 -- not a known variable star
21:25:27.48 +37:40:36.4 -- not a known variable star
21:25:47.96 +38:44:14.8 -- not a known variable star
21:25:52.28 +34:14:43.9 -- not a known variable star
21:25:56.52 +38:11:59.2 -- not a known variable star
21:26:05.34 +35:06:07.9 -- not a known variable star
21:26:10.16 +38:57:59.5 -- not a known variable star
21:26:11.09 +42:43:43.7 -- a known variable star
21:26:25.16 +35:51:25.5 -- not a known variable star
21:26:25.71 +40:35:04.0 -- not a known variable star
21:26:27.74 +35:10:57.9 -- a known variable star
21:26:28.37 +37:36:33.1 -- a known variable star
21:26:38.61 +39:47:22.1 -- not a known variable star
21:26:50.82 +42:27:02.6 -- not a known variable star
21:26:53.16 +37:31:50.2 -- not a known variable star
21:26:53.39 +40:39:04.3 -- not a known variable star
21:26:55.09 +38:03:54.1 -- not a known variable star
21:26:58.76 +38:06:04.9 -- not a known variable star
21:27:06.47 +33:44:08.5 -- a known variable star
21:27:09.80 +36:53:13.9 -- not a known variable star
21:27:12.32 +39:44:01.5 -- not a known variable star
21:27:27.41 +38:09:22.7 -- not a known variable star
21:27:28.52 +35:23:02.6 -- a known variable star
21:27:31.59 +35:50:08.1 -- not a known variable star
21:27:39.99 +41:28:15.9 -- not a known variable star
21:27:59.74 +37:32:17.8 -- not a known variable star
21:28:00.13 +36:42:32.1 -- not a known variable star
21:28:04.36 +43:01:07.6 -- not a known variable star
21:28:05.33 +38:26:58.1 -- not a known variable star
21:28:06.54 +36:36:22.2 -- not a known variable star
21:28:06.78 +39:56:16.0 -- a known variable star
21:28:11.68 +40:25:03.1 -- a known variable star
21:28:13.70 +33:56:53.8 -- not a known variable star
21:28:14.41 +42:51:46.0 -- not a known variable star
21:28:18.00 +34:05:00.0 -- not a known variable star
21:28:24.99 +39:10:02.1 -- not a known variable star
21:28:37.89 +35:33:42.3 -- not a known variable star
21:28:40.79 +39:00:17.9 -- not a known variable star
21:28:41.55 +42:35:38.9 -- a known variable star
21:28:43.59 +35:11:00.7 -- a known variable star
21:28:43.64 +35:42:00.9 -- not a known variable star
21:28:44.93 +38:10:24.2 -- not a known variable star
21:28:49.03 +41:29:04.0 -- not a known variable star
21:29:00.59 +35:14:11.5 -- not a known variable star
21:29:02.36 +41:37:46.7 -- a known variable star
21:29:04.95 +40:27:04.6 -- not a known variable star
21:29:06.42 +42:10:44.9 -- not a known variable star
21:29:08.03 +42:01:02.7 -- a known variable star
21:29:27.20 +34:33:19.8 -- not a known variable star
21:29:32.10 +33:48:17.3 -- not a known variable star
21:29:38.32 +39:05:20.9 -- not a known variable star
21:30:05.02 +40:57:00.0 -- not a known variable star
21:30:06.71 +42:42:51.2 -- not a known variable star
21:30:24.45 +39:13:33.0 -- not a known variable star
21:30:37.79 +42:45:58.2 -- not a known variable star
21:30:38.52 +36:36:07.3 -- not a known variable star
21:30:39.37 +38:36:13.0 -- not a known variable star
21:30:49.11 +38:57:23.2 -- not a known variable star
21:31:05.87 +41:04:08.3 -- not a known variable star
21:31:06.80 +39:46:47.2 -- not a known variable star
21:31:14.91 +38:46:29.7 -- a known variable star
21:31:17.20 +37:57:30.7 -- not a known variable star
21:31:28.06 +39:47:03.7 -- not a known variable star
21:31:29.67 +33:55:39.5 -- not a known variable star
21:31:39.14 +36:46:27.5 -- not a known variable star
21:32:05.87 +40:41:03.1 -- a known variable star
21:32:06.88 +39:41:52.2 -- not a known variable star
21:32:16.35 +41:10:14.6 -- a known variable star
21:32:24.91 +37:04:42.8 -- not a known variable star
21:32:26.27 +37:28:42.2 -- not a known variable star
21:32:28.08 +38:05:43.0 -- not a known variable star
21:32:31.54 +41:50:58.7 -- not a known variable star
21:32:41.02 +38:29:40.1 -- not a known variable star
21:32:48.30 +39:29:39.6 -- not a known variable star
21:33:08.65 +41:21:51.9 -- a known variable star
21:33:09.21 +37:05:56.5 -- not a known variable star
21:33:16.02 +41:46:48.1 -- not a known variable star
21:33:38.40 +34:07:28.0 -- not a known variable star
21:33:40.41 +40:44:24.3 -- not a known variable star
21:33:53.13 +33:18:17.1 -- not a known variable star
21:34:11.25 +40:41:03.1 -- not a known variable star
21:34:17.47 +36:20:30.1 -- not a known variable star
21:34:40.18 +37:29:31.8 -- not a known variable star
21:34:52.89 +37:58:12.8 -- not a known variable star
21:34:59.13 +39:59:54.0 -- not a known variable star
21:35:21.80 +41:16:18.5 -- not a known variable star
21:35:23.88 +36:47:17.3 -- not a known variable star
21:35:24.40 +36:45:52.6 -- not a known variable star
21:35:28.32 +41:43:14.3 -- not a known variable star
21:35:31.04 +33:55:25.7 -- a known variable star
21:35:50.10 +39:03:54.1 -- a known variable star
21:35:50.35 +40:48:09.1 -- not a known variable star
21:36:15.14 +40:02:53.3 -- not a known variable star
21:36:18.16 +40:03:04.6 -- not a known variable star
21:36:23.84 +37:34:30.9 -- not a known variable star
21:36:26.19 +42:23:45.7 -- not a known variable star
21:36:48.43 +38:51:41.5 -- not a known variable star
21:36:54.29 +40:36:45.6 -- not a known variable star
21:37:02.07 +39:22:40.0 -- a known variable star
21:37:34.51 +32:59:49.5 -- not a known variable star
21:37:35.64 +40:12:05.7 -- not a known variable star
21:37:42.98 +40:11:43.1 -- not a known variable star
21:37:44.49 +42:39:12.3 -- not a known variable star
21:37:50.58 +36:54:52.2 -- not a known variable star
21:37:54.69 +33:00:12.4 -- a known variable star
21:38:11.91 +37:42:54.7 -- not a known variable star
21:38:19.56 +39:47:35.3 -- not a known variable star
21:38:48.53 +41:18:14.6 -- not a known variable star
21:38:56.76 +37:31:12.5 -- not a known variable star
21:39:02.90 +40:22:35.9 -- not a known variable star
21:39:30.73 +37:21:41.9 -- not a known variable star
21:39:31.73 +40:39:06.9 -- not a known variable star
21:39:47.29 +42:43:07.2 -- not a known variable star
21:39:50.83 +41:51:15.2 -- not a known variable star
21:40:15.33 +37:50:20.7 -- not a known variable star
21:40:19.25 +38:45:41.7 -- not a known variable star
21:40:19.37 +35:38:56.5 -- not a known variable star
21:40:23.65 +39:00:27.7 -- not a known variable star
21:40:35.21 +39:13:32.1 -- not a known variable star
21:40:47.73 +38:06:20.2 -- not a known variable star
21:41:18.31 +41:17:54.2 -- a known variable star
21:41:20.41 +36:37:18.6 -- not a known variable star
21:41:27.40 +42:51:23.9 -- not a known variable star
21:41:50.86 +35:55:28.9 -- not a known variable star
21:42:06.01 +36:50:53.0 -- not a known variable star
21:42:23.05 +40:36:53.1 -- not a known variable star
21:42:23.52 +41:49:36.8 -- not a known variable star
21:42:31.17 +35:51:15.0 -- not a known variable star
21:42:46.31 +37:59:49.7 -- not a known variable star
21:43:03.17 +37:32:30.3 -- not a known variable star
21:43:09.61 +39:56:52.7 -- a known variable star
21:43:18.74 +42:12:53.6 -- not a known variable star
21:43:35.18 +37:22:30.0 -- a known variable star
21:43:36.58 +42:31:44.2 -- not a known variable star
21:43:42.41 +42:34:57.7 -- not a known variable star
21:43:55.49 +42:55:24.1 -- a known variable star
21:44:15.84 +42:45:31.0 -- not a known variable star
21:44:49.72 +36:56:53.9 -- not a known variable star
21:45:01.25 +42:15:60.0 -- not a known variable star
21:45:30.06 +40:39:22.2 -- not a known variable star
21:46:00.43 +37:21:18.7 -- not a known variable star
21:46:05.72 +42:50:03.3 -- not a known variable star
21:46:08.61 +35:33:30.2 -- not a known variable star
21:46:20.85 +36:51:37.6 -- not a known variable star
21:46:24.52 +41:13:01.9 -- a known variable star
21:46:34.06 +35:50:36.5 -- not a known variable star
21:46:41.17 +40:55:18.6 -- not a known variable star
21:46:53.87 +39:15:18.7 -- not a known variable star
21:48:46.98 +40:08:13.6 -- not a known variable star
21:48:47.70 +38:52:56.3 -- not a known variable star
21:49:04.94 +37:22:34.1 -- not a known variable star
21:49:31.96 +39:23:33.6 -- a known variable star
21:49:54.44 +34:54:43.5 -- not a known variable star
21:50:11.43 +35:33:08.1 -- a known variable star
21:50:17.58 +42:04:56.8 -- a known variable star
21:50:32.90 +33:17:12.9 -- not a known variable star
21:50:34.17 +37:11:04.4 -- not a known variable star
21:50:40.28 +40:44:27.7 -- not a known variable star
21:50:49.89 +33:01:37.9 -- a known variable star
21:51:38.10 +43:02:19.3 -- not a known variable star
21:52:14.88 +36:58:29.7 -- not a known variable star
21:52:16.26 +42:41:08.0 -- not a known variable star
21:52:59.99 +33:25:12.1 -- not a known variable star
21:53:17.43 +42:34:35.4 -- not a known variable star
21:53:19.50 +34:36:59.1 -- not a known variable star
21:53:37.45 +42:42:28.2 -- not a known variable star
21:54:17.19 +36:52:11.4 -- not a known variable star
21:54:33.42 +35:50:15.0 -- a known variable star
21:54:45.67 +38:18:18.0 -- not a known variable star
21:55:25.46 +41:56:48.8 -- not a known variable star
21:55:49.52 +34:16:12.7 -- not a known variable star
21:56:00.37 +37:10:55.8 -- not a known variable star
21:56:08.18 +40:50:21.0 -- not a known variable star
21:56:20.29 +42:31:29.4 -- not a known variable star
21:56:29.02 +36:52:32.3 -- not a known variable star
21:56:32.95 +38:17:22.8 -- not a known variable star
21:56:34.36 +37:00:25.9 -- not a known variable star
21:56:49.58 +42:13:05.3 -- not a known variable star
21:57:38.14 +32:57:13.0 -- not a known variable star
21:57:39.23 +41:47:19.7 -- not a known variable star
21:57:59.24 +41:37:13.3 -- not a known variable star
21:58:13.38 +38:26:14.2 -- not a known variable star
21:58:49.37 +40:28:42.2 -- not a known variable star
21:59:30.86 +42:08:23.4 -- not a known variable star
21:59:59.93 +38:42:23.1 -- a known variable star
22:00:11.18 +39:37:38.7 -- not a known variable star
22:00:15.47 +42:40:23.2 -- not a known variable star
22:00:32.83 +39:39:03.1 -- not a known variable star
22:01:03.93 +41:04:56.1 -- a known variable star
22:01:06.44 +42:14:35.8 -- not a known variable star
22:01:07.92 +39:15:18.7 -- not a known variable star
22:01:22.36 +40:55:08.1 -- not a known variable star
22:01:26.89 +38:07:17.1 -- not a known variable star
22:01:57.33 +35:42:30.3 -- not a known variable star
22:02:04.51 +37:45:26.1 -- not a known variable star
22:02:09.38 +41:51:02.7 -- not a known variable star
22:02:13.82 +41:47:07.6 -- not a known variable star
22:02:22.40 +41:34:46.0 -- not a known variable star
22:02:27.71 +42:04:01.9 -- not a known variable star
22:04:36.81 +38:54:14.7 -- not a known variable star
22:05:01.96 +41:27:41.8 -- not a known variable star
22:05:11.01 +42:22:39.9 -- not a known variable star
22:05:11.22 +41:31:52.7 -- not a known variable star
22:05:53.83 +33:29:13.6 -- not a known variable star
22:06:26.75 +38:35:58.2 -- not a known variable star
22:06:46.45 +39:39:05.9 -- not a known variable star
22:06:54.81 +41:38:24.7 -- not a known variable star
22:07:43.00 +39:34:56.3 -- not a known variable star
22:07:43.26 +37:37:03.4 -- not a known variable star
22:07:49.45 +33:25:38.3 -- not a known variable star
22:08:04.65 +35:52:50.9 -- not a known variable star
22:08:32.91 +35:58:48.5 -- not a known variable star
22:09:11.24 +36:46:05.1 -- not a known variable star
22:09:13.49 +39:15:45.0 -- not a known variable star
22:09:21.19 +33:46:49.3 -- not a known variable star
22:09:23.69 +40:29:36.8 -- not a known variable star
22:09:31.96 +42:04:29.4 -- not a known variable star
22:09:56.43 +39:05:39.8 -- not a known variable star
22:10:15.65 +41:33:59.3 -- not a known variable star
22:11:18.63 +39:15:04.6 -- not a known variable star
22:12:04.42 +37:38:52.8 -- not a known variable star
22:12:21.99 +33:37:10.3 -- not a known variable star
22:12:22.91 +41:42:04.4 -- not a known variable star
22:12:26.42 +40:34:53.0 -- not a known variable star
22:13:03.48 +38:28:18.8 -- not a known variable star
22:13:08.46 +40:02:52.1 -- not a known variable star
22:14:09.47 +38:28:27.7 -- a known variable star
22:15:17.49 +39:47:51.6 -- not a known variable star
22:15:17.88 +37:28:35.3 -- not a known variable star
22:15:54.18 +37:58:56.1 -- not a known variable star
22:17:10.57 +41:19:17.1 -- not a known variable star
22:17:24.47 +38:35:02.3 -- not a known variable star
22:17:25.04 +42:04:44.7 -- not a known variable star
22:17:45.88 +39:00:20.5 -- not a known variable star
22:18:25.69 +41:03:50.0 -- a known variable star
22:18:47.95 +40:40:39.3 -- a known variable star
22:19:20.15 +40:03:19.4 -- not a known variable star
22:19:47.33 +42:24:09.0 -- not a known variable star
22:20:24.64 +41:35:26.1 -- not a known variable star
22:20:30.72 +33:13:11.8 -- not a known variable star
22:20:30.94 +33:33:35.0 -- a known variable star
22:20:33.29 +42:19:01.7 -- not a known variable star
22:20:44.67 +42:23:07.7 -- not a known variable star
22:21:09.27 +38:20:25.4 -- not a known variable star
22:21:12.77 +33:36:39.2 -- not a known variable star
22:21:21.34 +41:17:35.6 -- not a known variable star
22:21:24.16 +41:17:43.9 -- a known variable star
22:21:24.83 +40:44:14.1 -- not a known variable star
22:21:26.07 +42:04:44.1 -- not a known variable star
22:21:42.03 +36:19:16.6 -- not a known variable star
22:21:42.26 +40:38:49.2 -- not a known variable star
22:21:51.89 +38:05:41.0 -- not a known variable star
22:22:07.59 +40:53:07.5 -- not a known variable star
22:22:30.47 +41:47:35.7 -- not a known variable star
22:22:34.15 +40:52:05.2 -- not a known variable star
22:22:57.31 +41:08:15.2 -- not a known variable star
22:23:00.35 +33:22:31.9 -- not a known variable star
22:23:06.22 +41:02:00.8 -- a known variable star
22:23:25.16 +41:54:05.1 -- not a known variable star
22:23:32.73 +35:41:57.4 -- not a known variable star
22:23:37.34 +38:47:39.1 -- not a known variable star
22:23:41.87 +34:37:03.3 -- not a known variable star
22:23:44.27 +32:54:14.5 -- a known variable star
22:23:50.38 +40:10:59.7 -- not a known variable star
22:23:57.60 +41:47:31.3 -- not a known variable star
22:24:00.62 +40:01:13.8 -- not a known variable star
22:24:01.20 +39:08:02.8 -- not a known variable star
22:24:04.86 +41:24:51.1 -- not a known variable star
22:24:05.20 +39:13:30.0 -- a known variable star
22:24:14.06 +41:20:03.0 -- not a known variable star
22:24:21.88 +37:53:04.8 -- not a known variable star
22:24:29.96 +39:20:53.4 -- not a known variable star
22:24:31.98 +41:49:20.1 -- a known variable star
22:24:39.80 +40:04:40.5 -- not a known variable star
22:24:43.50 +41:45:09.0 -- not a known variable star
22:24:47.11 +40:38:54.7 -- not a known variable star
22:24:47.79 +41:23:34.1 -- a known variable star
22:25:02.35 +38:38:36.5 -- not a known variable star
22:25:10.79 +41:11:46.2 -- not a known variable star
22:25:36.46 +40:51:52.1 -- not a known variable star
22:25:38.23 +42:04:05.8 -- not a known variable star
22:25:38.96 +39:59:37.6 -- not a known variable star
22:25:57.18 +40:25:48.2 -- a known variable star
22:26:17.45 +40:38:22.7 -- not a known variable star
22:26:22.35 +40:13:20.3 -- not a known variable star
22:26:23.92 +39:12:21.1 -- a known variable star
22:26:27.62 +39:49:37.8 -- not a known variable star
22:26:30.26 +42:15:27.1 -- not a known variable star
22:26:35.03 +36:53:06.5 -- a known variable star
22:26:44.89 +40:34:42.4 -- not a known variable star
22:26:47.99 +39:55:16.8 -- not a known variable star
22:26:53.22 +41:24:28.4 -- not a known variable star
22:27:00.92 +41:35:40.0 -- not a known variable star
22:27:04.57 +38:45:58.5 -- not a known variable star
22:27:09.21 +40:20:16.7 -- not a known variable star
22:27:14.92 +42:09:27.2 -- not a known variable star
22:27:15.22 +40:20:02.7 -- not a known variable star
22:27:32.23 +40:12:33.7 -- not a known variable star
22:27:39.15 +41:18:21.0 -- not a known variable star
22:27:39.56 +42:05:42.1 -- not a known variable star
22:27:43.44 +38:34:06.4 -- a known variable star
22:27:53.50 +39:12:46.3 -- not a known variable star
22:27:59.83 +41:57:08.5 -- not a known variable star
22:28:16.73 +41:56:38.2 -- a known variable star
22:28:36.87 +41:59:19.8 -- not a known variable star
22:28:37.12 +40:06:52.2 -- not a known variable star
22:28:39.45 +41:36:50.0 -- a known variable star
22:28:45.72 +41:44:04.0 -- not a known variable star
22:29:17.65 +41:28:02.2 -- not a known variable star
22:29:26.94 +40:50:02.5 -- a known variable star
22:29:53.35 +41:26:00.2 -- not a known variable star
Found 497 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
583 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 583 (excluding asteroids and hot pixels, 497 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)2461185.84693154 -observatory V36
04:59:58.17 +24:28:40.7 Mercury (-1.2mag)
06:31:31.56 +25:01:11.5 Venus (-3.9mag)
02:09:39.35 +12:20:53.7 Mars (1.3mag)
07:37:20.53 +21:57:52.7 Jupiter (-1.9mag)
00:45:00.93 +02:24:14.8 Saturn (0.9mag)
03:56:51.94 +20:15:42.6 Uranus (5.8mag)
00:15:09.62 +00:11:09.4 Neptune (7.8mag)
20:33:57.93 -22:59:48.3 Pluto (14.5mag)
11:40:25.45 -00:47:05.0 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 363 May 25 04:30 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461185.84693154:
07:37:27.82 +21:57:34.1 Io (5.9mag)
07:37:27.83 +21:57:34.6 Europa (6.1mag)
07:37:04.91 +21:58:37.3 Ganymede (5.5mag)
07:37:06.43 +21:58:23.8 Callisto (6.7mag)
07:38:28.74 +21:34:17.3 Himalia (15.5mag)
07:37:17.93 +21:58:00.7 Thebe (16.5mag)
07:38:48.05 +21:55:54.6 Elara (17.5mag)
07:38:45.42 +22:17:05.0 Pasiphae (17.7mag)
07:44:29.57 +21:58:39.2 Carme (18.8mag)
00:44:59.32 +02:23:58.4 Titan (8.7mag)
00:44:59.59 +02:24:29.9 Rhea (10.0mag)
00:45:22.00 +02:24:12.4 Iapetus (11.4mag)
00:45:16.27 +02:24:11.2 Hyperion (14.7mag)
00:45:59.51 +02:28:08.7 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 04:30 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461185.84693154:
17:15:52.57 -33:12:08.6 JWST
19:56:42.24 -02:33:16.7 Chandra
20:12:51.27 +25:42:25.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 04:30 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461185.84693154 -observatory V36
13:21:29.31 -27:08:45.7 14.4mag D/1884 O1 (Barnard)
06:35:54.63 +30:41:36.1 15.7mag D/1886 K1 (Brooks)
15:27:03.64 +01:18:51.0 14.6mag D/1895 Q1 (Swift)
05:26:50.24 +24:37:05.8 17.2mag D/1918 W1 (Schorr)
09:25:28.62 +15:18:12.2 17.9mag P/2009 WX51 (Catalina)
18:51:23.46 -31:35:29.7 13.7mag P/2010 H2 (Vales)
05:40:05.64 -68:17:05.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:03.70 +31:47:55.1 17.4mag C/2017 K2 (PANSTARRS)
17:20:10.64 +14:29:15.2 17.7mag C/2021 G2 (ATLAS)
23:14:36.51 +31:00:34.7 17.2mag C/2022 E2 (ATLAS)
05:16:58.73 +26:50:51.3 16.4mag C/2022 N2 (PANSTARRS)
09:20:26.58 +31:30:59.3 16.5mag C/2022 QE78 (ATLAS)
08:43:37.88 +03:09:59.4 17.6mag C/2022 R6 (PANSTARRS)
18:36:51.32 +21:10:10.7 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:47.79 -11:02:34.2 17.5mag P/2023 B1 (PANSTARRS)
22:16:09.49 +65:36:14.3 17.7mag C/2023 H5 (Lemmon)
18:18:56.46 -05:28:15.3 13.7mag C/2023 R1 (PANSTARRS)
13:42:49.78 +85:58:02.2 17.9mag C/2023 X2 (Lemmon)
06:52:25.34 +63:54:27.4 17.6mag C/2024 A1 (ATLAS)
06:25:32.19 +26:22:49.8 13.1mag C/2024 E1 (Wierzchos)
15:48:34.78 +12:06:46.4 17.3mag C/2024 G6 (ATLAS)
20:20:06.63 +26:55:00.3 14.1mag C/2024 J3 (ATLAS)
04:04:08.96 -17:17:30.6 16.1mag C/2024 T5 (ATLAS)
05:52:52.25 +36:58:07.4 17.9mag C/2025 J1 (Borisov)
11:46:43.76 +53:21:30.1 16.9mag C/2025 L1 (ATLAS)
06:23:14.05 -10:07:39.6 12.5mag C/2025 R3 (PANSTARRS)
12:41:05.62 +04:36:13.2 17.2mag C/2025 Y1 (ATLAS)
01:34:38.60 +42:18:30.5 15.7mag C/2026 B2 (Sun-Gao)
11:10:31.03 -09:22:17.9 16.2mag A/2026 E1
19:58:06.53 -08:07:20.6 9.5mag 10P/Tempel
14:19:08.02 -02:27:08.4 17.6mag 24P/Schaumasse
10:59:37.46 -00:51:51.1 15.9mag 29P/Schwassmann-Wachmann
10:50:46.15 -02:34:20.3 17.7mag 43P/Wolf-Harrington
02:50:09.39 +23:42:55.9 17.6mag 47P/Ashbrook-Jackson
08:30:28.35 +27:35:27.7 16.9mag 63P/Wild
00:14:03.55 -07:23:27.7 15.7mag 65P/Gunn
05:59:00.03 +31:32:38.6 16.5mag 76P/West-Kohoutek-Ikemura
02:35:58.93 +15:15:46.1 13.9mag 78P/Gehrels
00:49:10.06 +01:36:45.5 15.3mag 88P/Howell
04:10:06.18 +28:49:56.5 15.1mag 93P/Lovas
02:05:13.39 +25:11:48.2 18.0mag 114P/Wiseman-Skiff
06:18:04.31 +33:19:49.9 15.7mag 123P/West-Hartley
09:26:33.70 +20:38:03.0 16.4mag 124P/Mrkos
03:36:14.08 +18:13:18.5 16.4mag 128P/Shoemaker-Holt
04:05:54.10 +18:17:30.7 17.7mag 131P/Mueller
04:54:38.42 +19:40:02.2 12.9mag 141P/Machholz
04:57:19.91 +16:15:19.7 12.8mag 141P-A/Machholz
03:42:05.25 +13:31:02.1 10.6mag 141P-D/Machholz
02:47:34.56 -26:47:20.1 17.3mag 161P/Hartley-IRAS
02:57:18.22 +17:51:11.8 14.9mag 162P/SidingSpring
19:34:27.39 -01:54:32.4 17.6mag 169P/NEAT
17:02:59.19 -09:25:52.3 16.2mag 235P/LINEAR
07:03:07.50 +35:52:35.6 17.3mag 240P/NEAT
23:56:24.49 -08:05:41.3 16.8mag 260P/McNaught
03:27:53.19 +29:44:48.6 17.7mag 295P/LINEAR
21:56:48.78 -28:33:21.4 17.7mag 320P/McNaught
15:22:11.76 +08:21:51.9 17.4mag 391P/Kowalski
07:56:36.94 +21:03:15.2 17.8mag 450P/LONEOS
06:37:24.12 +42:38:31.8 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 04:30 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 04:30 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 04:30 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
13:16:20.230 +02:48:58.63 AT 2026mwp 2026-05-03.68 21.84
13:17:52.545 -50:04:09.72 AT 2026mwo 2026-04-12.49 19.69
11:28:16.230 +42:22:52.41 AT 2026mwn 2026-05-12.89 19.9
-rw-r--r-- 1 apache apache 30K May 25 04:30 tns_transients_list.txt
