This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO
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 11.3407 2461171.8407 12.43 21:37:22.59 +37:20:59.2
85.57248 -11.07076 galactic Cyg Second-epoch detections are separated by 1.8" 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 | target | 21:37:22.59 +37:20:59.2 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:22.59 +37:20:59.2: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:22.59 +37:20:59.2: 14.40 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.27 21:56:43.79 +40:46:35.1
90.74896 -10.93105 galactic Cyg Second-epoch detections are separated by 1.0" 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 | 21:56:43.79 +40:46:35.1 (user input) | T | P | (position from user input) J-Ks=0.563+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:43.79 +40:46:35.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:43.79 +40:46:35.1: 14.53 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.53 +/- 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,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.20 21:32:46.06 +37:06:20.3
84.72156 -10.62037 galactic Cyg Second-epoch detections are separated by 3.1" 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 | 21:32:46.06 +37:06:20.3 (user input) | T | P | (position from user input) J-Ks=0.194+/-0.069 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:46.06 +37:06:20.3: 12.59 +/- 0.16 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:46.06 +37:06:20.3: 14.27 +/- 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
target,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.31 21:39:49.97 +38:35:47.4
86.79307 -10.47842 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 | 21:39:49.97 +38:35:47.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:49.97 +38:35:47.4: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:49.97 +38:35:47.4: 15.10 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.10 +/- 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,2461171.8407,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.23 21:49:23.73 +39:00:35.9
88.49682 -11.39683 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 | target | 21:49:23.73 +39:00:35.9 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:23.73 +39:00:35.9: 12.55 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:23.73 +39:00:35.9: 13.98 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.28 21:29:18.50 +38:46:45.3
85.39920 -8.94104 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 21:29:18.50 +38:46:45.3 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:18.50 +38:46:45.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:18.50 +38:46:45.3: 14.53 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.53 +/- 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,2461171.8407,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.35 21:35:59.60 +40:25:24.8
87.48890 -8.63028 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 J324.0032+40.4230 | 21:35:59.60 +40:25:24.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:59.60 +40:25:24.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:59.60 +40:25:24.8: 14.52 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.0032+40.4230,2461171.8407,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0032+40.4230 20260511.3407 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 11.3407 2461171.8407 12.19 21:36:56.47 +36:30:11.3
84.91974 -11.63184 galactic Cyg Second-epoch detections are separated by 1.3" and 7.4 pix
The object was found in VSX 2" Gaia DR3 1951138324711432192
Type: ROT
# Max. Min./Amp. JD0 Period
14.560 G 14.590 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:56.47 +36:30:11.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:56.47 +36:30:11.3: 14.30 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951138324711432192,2461171.8407,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951138324711432192 20260511.3407 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 11.3407 2461171.8407 12.16 21:47:21.70 +36:09:48.3
86.28208 -13.29016 galactic Cyg Second-epoch detections are separated by 2.9" 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 | target | 21:47:21.70 +36:09:48.3 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:21.70 +36:09:48.3: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:21.70 +36:09:48.3: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.11 21:38:52.80 +38:18:22.9
86.45413 -10.56751 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 | ATO J324.7082+38.3006 | 21:38:52.80 +38:18:22.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.373+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:52.80 +38:18:22.9: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:52.80 +38:18:22.9: 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
ATO J324.7082+38.3006,2461171.8407,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7082+38.3006 20260511.3407 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 11.3407 2461171.8407 12.29 21:34:54.35 +35:45:42.5
84.09528 -11.89062 galactic Cyg Second-epoch detections are separated by 2.4" 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 | ATO J323.7303+35.7597 | 21:34:54.35 +35:45:42.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:54.35 +35:45:42.5: 13.45 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:54.35 +35:45:42.5: 14.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.7303+35.7597,2461171.8407,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.7303+35.7597 20260511.3407 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 11.3407 2461171.8407 12.14 21:49:05.46 +40:42:33.5
89.56989 -10.06280 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 21:49:05.46 +40:42:33.5 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.415+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:05.46 +40:42:33.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:05.46 +40:42:33.5: 14.24 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.24 +/- 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,2461171.8407,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.29 21:37:37.57 +39:15:52.6
86.92806 -9.69556 galactic Cyg Second-epoch detections are separated by 0.3" and 7.1 pix
The object was found in VSX 2" Gaia DR3 1953934971197732096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.670 G 14.700 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:37.57 +39:15:52.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:37.57 +39:15:52.6: 14.68 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1953934971197732096,2461171.8407,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1953934971197732096 20260511.3407 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 11.3407 2461171.8407 12.18 21:55:24.97 +39:42:13.4
89.86261 -11.60774 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 | 21:55:24.97 +39:42:13.4 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:24.97 +39:42:13.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:24.97 +39:42:13.4: 14.36 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.02 21:40:39.53 +36:27:53.0
85.45477 -12.16645 galactic Cyg Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX24" Gaia DR3 1951099846104858240
Type: ROT
# Max. Min./Amp. JD0 Period
14.420 G 14.450 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:39.53 +36:27:53.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:39.53 +36:27:53.0: 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
Gaia DR3 1951099846104858240,2461171.8407,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951099846104858240 20260511.3407 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 11.3407 2461171.8407 11.94 21:57:32.70 +38:48:28.7
89.61370 -12.56323 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 | ATO J329.3824+38.7999 | 21:57:32.70 +38:48:28.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:32.70 +38:48:28.7: 12.94 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:32.70 +38:48:28.7: 14.34 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.3824+38.7999,2461171.8407,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.3824+38.7999 20260511.3407 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 11.3407 2461171.8407 12.11 21:45:04.66 +40:22:24.7
88.76035 -9.82138 galactic Cyg Second-epoch detections are separated by 1.6" 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 J326.2785+40.3739 | 21:45:04.66 +40:22:24.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:04.66 +40:22:24.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:04.66 +40:22:24.7: 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
ATO J326.2785+40.3739,2461171.8407,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.2785+40.3739 20260511.3407 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 11.3407 2461171.8407 11.96 21:55:46.17 +35:47:05.8
87.36424 -14.68091 galactic Peg 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 | 21:55:46.17 +35:47:05.8 (user input) | T | P | (position from user input) J-Ks=0.596+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:46.17 +35:47:05.8: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:46.17 +35:47:05.8: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.20 21:31:26.61 +39:18:37.8
86.07431 -8.84510 galactic Cyg Second-epoch detections are separated by 0.9" and 7.0 pix
The object was found in VSX23" Gaia DR3 1964409090764606080
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.680 G 14.730 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:26.61 +39:18:37.8: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:26.61 +39:18:37.8: 14.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1964409090764606080,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964409090764606080 20260511.3407 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 11.3407 2461171.8407 12.12 21:38:15.65 +36:10:02.1
84.88509 -12.05882 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 | ATO J324.5657+36.1671 | 21:38:15.65 +36:10:02.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.383+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:15.65 +36:10:02.1: 13.62 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:15.65 +36:10:02.1: 14.20 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.15 +/- 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 J324.5657+36.1671,2461171.8407,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5657+36.1671 20260511.3407 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 11.3407 2461171.8407 12.13 21:46:11.75 +36:11:01.4
86.11415 -13.11976 galactic Cyg 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 | Gaia DR3 1952347203385198464 | 21:46:12.42 +36:10:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.556+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:11.75 +36:11:01.4: 12.53 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:11.75 +36:11:01.4: 14.24 +/- 0.11 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
Gaia DR3 1952347203385198464,2461171.8407,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952347203385198464 20260511.3407 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 11.3407 2461171.8407 12.20 21:40:23.68 +39:00:28.4
87.15606 -10.24664 galactic Cyg Second-epoch detections are separated by 0.2" 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 | target | 21:40:23.68 +39:00:28.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:23.68 +39:00:28.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:23.68 +39:00:28.4: 14.42 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.13 21:36:18.88 +36:34:10.5
84.87215 -11.49739 galactic Cyg Second-epoch detections are separated by 3.4" 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 | ATO J324.0889+36.5679 | 21:36:18.88 +36:34:10.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:18.88 +36:34:10.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:18.88 +36:34:10.5: 14.98 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.98 +/- 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 J324.0889+36.5679,2461171.8407,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0889+36.5679 20260511.3407 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 11.3407 2461171.8407 12.08 21:30:30.86 +38:24:14.2
85.30698 -9.37474 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 J322.6295+38.4028 | 21:30:30.86 +38:24:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.257+/- (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:30.86 +38:24:14.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:30.86 +38:24:14.2: 14.69 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.69 +/- 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 J322.6295+38.4028,2461171.8407,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.6295+38.4028 20260511.3407 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 11.3407 2461171.8407 12.25 21:41:16.01 +42:07:07.3
89.38062 -8.03724 galactic Cyg Second-epoch detections are separated by 5.1" 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 | Large-amplitude variable Gaia DR2 1966629073452261248 | 21:41:16.01 +42:07:07.3 (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=0.512+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:16.01 +42:07:07.3: 13.29 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:16.01 +42:07:07.3: 14.55 +/- 0.17 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
Large-amplitude variable Gaia DR2 1966629073452261248,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1966629073452261248 20260511.3407 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 11.3407 2461171.8407 11.83 21:51:31.73 +37:29:41.7
87.82204 -12.82354 galactic Cyg Second-epoch detections are separated by 2.6" 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 J327.8782+37.4956 | 21:51:31.73 +37:29:41.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-0.041 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:31.73 +37:29:41.7: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:31.73 +37:29:41.7: 13.86 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.8782+37.4956,2461171.8407,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.8782+37.4956 20260511.3407 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 11.3407 2461171.8407 12.05 21:36:44.12 +39:54:03.5
87.23614 -9.11073 galactic Cyg Second-epoch detections are separated by 2.2" 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 | target | 21:36:44.12 +39:54:03.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.862+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:44.12 +39:54:03.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:44.12 +39:54:03.5: 14.06 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.10 21:31:11.07 +35:03:50.6
83.04256 -11.86881 galactic Cyg 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 | 21:31:11.07 +35:03:50.6 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:11.07 +35:03:50.6: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:11.07 +35:03:50.6: 14.72 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.72 +/- 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,2461171.8407,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.00 21:38:44.15 +35:57:37.8
84.81355 -12.27577 galactic Cyg Second-epoch detections are separated by 1.3" and 7.4 pix
The object was found in VSX18" Gaia DR3 1951062222190619520
Type: ROT
# Max. Min./Amp. JD0 Period
14.520 G 14.550 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:44.15 +35:57:37.8: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:44.15 +35:57:37.8: 14.04 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951062222190619520,2461171.8407,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951062222190619520 20260511.3407 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 11.3407 2461171.8407 12.01 21:39:43.24 +34:48:32.9
84.16343 -13.25756 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 | target | 21:39:43.24 +34:48:32.9 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:43.24 +34:48:32.9: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:43.24 +34:48:32.9: 14.13 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.06 21:27:52.85 +41:24:14.8
87.04422 -6.86504 galactic Cyg Second-epoch detections are separated by 1.5" and 7.2 pix
The object was found in VSX23" Gaia DR3 1967073306221380224
Type: E
# Max. Min./Amp. JD0 Period
17.820 G 18.010 G 4.233780000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:52.85 +41:24:14.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:52.85 +41:24:14.8: 14.65 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.65 +/- 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 1967073306221380224,2461171.8407,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967073306221380224 20260511.3407 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 11.3407 2461171.8407 11.91 21:43:44.31 +34:49:09.2
84.79694 -13.80603 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 | 21:43:44.31 +34:49:09.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:44.31 +34:49:09.2: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:44.31 +34:49:09.2: 14.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.67 +/- 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,2461171.8407,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.15 21:27:27.91 +39:54:37.7
85.93768 -7.88137 galactic Cyg Second-epoch detections are separated by 3.8" 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 | ATO J321.8597+39.9073 | 21:27:27.91 +39:54:37.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.918+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:27.91 +39:54:37.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:27.91 +39:54:37.7: 13.79 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.8597+39.9073,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8597+39.9073 20260511.3407 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 11.3407 2461171.8407 11.96 21:50:55.91 +34:03:35.1
85.42653 -15.35687 galactic Peg Second-epoch detections are separated by 1.5" 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 | 21:50:55.91 +34:03:35.1 (user input) | T | P | (position from user input) J-Ks=0.309+/-0.040 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:55.91 +34:03:35.1: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:55.91 +34:03:35.1: 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,2461171.8407,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.71 21:55:39.57 +36:53:20.5
88.07233 -13.81576 galactic Cyg Second-epoch detections are separated by 2.2" 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 | target | 21:55:39.57 +36:53:20.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:39.57 +36:53:20.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:39.57 +36:53:20.5: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461171.8407,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.92 21:44:37.46 +38:02:16.4
87.12781 -11.52118 galactic Cyg 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 | 21:44:37.46 +38:02:16.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:37.46 +38:02:16.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:37.46 +38:02:16.4: 14.06 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.81 22:08:32.33 +35:58:54.1
89.59282 -16.13428 galactic Lac 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 | 22:08:32.33 +35:58:54.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:08:32.33 +35:58:54.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:08:32.33 +35:58:54.1: 14.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.88 21:51:26.68 +38:24:23.9
88.41075 -12.11566 galactic Cyg Second-epoch detections are separated by 3.4" 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 | 21:51:26.68 +38:24:23.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.483+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:26.68 +38:24:23.9: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:26.68 +38:24:23.9: 13.93 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461171.8407,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.04 21:36:58.25 +37:51:36.9
85.86558 -10.64161 galactic Cyg Second-epoch detections are separated by 0.8" 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 | ATO J324.2508+37.8632 | 21:36:58.25 +37:51:36.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.640+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:58.25 +37:51:36.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:58.25 +37:51:36.9: 14.50 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2508+37.8632,2461171.8407,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2508+37.8632 20260511.3407 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 11.3407 2461171.8407 11.86 22:06:56.03 +41:38:43.3
92.83813 -11.41765 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 | 22:06:56.03 +41:38:43.3 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:56.03 +41:38:43.3: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:56.03 +41:38:43.3: 14.56 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.78 21:48:31.20 +41:08:42.7
89.77216 -9.66041 galactic Cyg Second-epoch detections are separated by 0.2" 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 J327.1211+41.1406 | 21:48:31.20 +41:08:42.7 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:31.20 +41:08:42.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:31.20 +41:08:42.7: 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 J327.1211+41.1406,2461171.8407,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1211+41.1406 20260511.3407 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 11.3407 2461171.8407 11.79 22:05:37.24 +38:57:41.5
90.98056 -13.41136 galactic Lac 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 | target | 22:05:37.24 +38:57:41.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:37.24 +38:57:41.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:37.24 +38:57:41.5: 13.62 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461171.8407,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.88 21:38:33.76 +37:39:20.4
85.95994 -11.00528 galactic Cyg Second-epoch detections are separated by 0.2" 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 | target | 21:38:33.76 +37:39:20.4 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.080 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:33.76 +37:39:20.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:33.76 +37:39:20.4: 13.86 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.88 21:40:15.50 +37:50:19.7
86.33801 -11.09589 galactic Cyg Second-epoch detections are separated by 1.0" 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 | ATO J325.0657+37.8384 | 21:40:15.50 +37:50:19.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:15.50 +37:50:19.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:15.50 +37:50:19.7: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0657+37.8384,2461171.8407,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0657+37.8384 20260511.3407 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 11.3407 2461171.8407 11.91 21:38:51.21 +41:31:56.0
88.64725 -8.17487 galactic Cyg Second-epoch detections are separated by 0.7" and 6.9 pix
The object was found in VSX 3" ZTF J213851.32+413159.0
Type: SR
# Max. Min./Amp. JD0 Period
14.305 r Y 0.585 r 2458472.85290 80.340818400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:51.21 +41:31:56.0: 13.23 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:51.21 +41:31:56.0: 13.92 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213851.32+413159.0,2461171.8407,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213851.32+413159.0 20260511.3407 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 11.3407 2461171.8407 11.73 22:00:34.77 +38:25:34.0
89.84462 -13.23142 galactic Lac Second-epoch detections are separated by 1.5" 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 | target | 22:00:34.77 +38:25:34.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.396+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:34.77 +38:25:34.0: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:34.77 +38:25:34.0: 14.47 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.47 +/- 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,2461171.8407,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.76 21:38:21.00 +42:10:14.8
89.00887 -7.63798 galactic Cyg Second-epoch detections are separated by 2.4" 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 | 21:38:21.00 +42:10:14.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:21.00 +42:10:14.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:21.00 +42:10:14.8: 13.94 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461171.8407,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.03 21:32:45.17 +38:02:04.6
85.37042 -9.94553 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 | 21:32:45.17 +38:02:04.6 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.701+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:45.17 +38:02:04.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:45.17 +38:02:04.6: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461171.8407,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.00 21:40:56.29 +40:31:32.9
88.26333 -9.18650 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 | Gaia DR3 1954384770230429056 | 21:40:56.33 +40:30:51.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:56.29 +40:31:32.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:56.29 +40:31:32.9: 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
Gaia DR3 1954384770230429056,2461171.8407,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954384770230429056 20260511.3407 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 11.3407 2461171.8407 11.77 21:53:53.72 +40:08:53.0
89.91910 -11.07918 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 21:53:53.72 +40:08:53.0 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:53.72 +40:08:53.0: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:53.72 +40:08:53.0: 14.50 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.50 +/- 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,2461171.8407,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.73 21:41:28.53 +41:30:43.3
89.00341 -8.51705 galactic Cyg 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 J325.3764+41.5141 | 21:41:28.53 +41:30:43.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.429+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:28.53 +41:30:43.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:28.53 +41:30:43.3: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3764+41.5141,2461171.8407,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3764+41.5141 20260511.3407 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 11.3407 2461171.8407 11.64 22:10:45.38 +40:14:53.4
92.58481 -12.97063 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 | target | 22:10:45.38 +40:14:53.4 (user input) | T | P | (position from user input) J-Ks=0.703+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:45.38 +40:14:53.4: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:45.38 +40:14:53.4: 14.02 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.63 21:55:57.22 +40:10:24.0
90.24616 -11.30800 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 | ATO J328.9858+40.1754 | 21:55:57.22 +40:10:24.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.373+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:57.22 +40:10:24.0: 13.07 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:57.22 +40:10:24.0: 13.88 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J328.9858+40.1754,2461171.8407,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9858+40.1754 20260511.3407 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 11.3407 2461171.8407 11.54 21:43:23.74 +33:45:12.7
84.00523 -14.54868 galactic Cyg Second-epoch detections are separated by 1.6" 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 | target | 21:43:23.74 +33:45:12.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:23.74 +33:45:12.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:23.74 +33:45:12.7: 13.13 +/- 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
target,2461171.8407,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.78 21:38:23.56 +40:06:15.1
87.61229 -9.17493 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 | Gaia DR3 1966007123531818496 | 21:38:26.69 +40:06:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.663+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:23.56 +40:06:15.1: 13.19 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:23.56 +40:06:15.1: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 1966007123531818496,2461171.8407,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966007123531818496 20260511.3407 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 11.3407 2461171.8407 11.51 22:04:27.90 +38:05:25.5
90.25063 -13.96541 galactic Lac 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 | target | 22:04:27.90 +38:05:25.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.688+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:04:27.90 +38:05:25.5: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:04:27.90 +38:05:25.5: 13.89 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461171.8407,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.56 21:28:22.20 +41:32:01.4
87.20131 -6.83552 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 | ATO J322.0893+41.5337 | 21:28:22.20 +41:32:01.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:22.20 +41:32:01.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:22.20 +41:32:01.4: 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
ATO J322.0893+41.5337,2461171.8407,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0893+41.5337 20260511.3407 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 11.3407 2461171.8407 11.82 21:35:26.51 +41:08:48.9
87.90711 -8.02786 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 | ATO J323.8637+41.1463 | 21:35:26.51 +41:08:48.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:26.51 +41:08:48.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:26.51 +41:08:48.9: 13.58 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8637+41.1463,2461171.8407,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8637+41.1463 20260511.3407 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 11.3407 2461171.8407 11.61 21:36:48.40 +35:29:07.4
84.18886 -12.35672 galactic Cyg Second-epoch detections are separated by 3.3" 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 J324.1949+35.4853 | 21:36:48.40 +35:29:07.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.672+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:48.40 +35:29:07.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:48.40 +35:29:07.4: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.1949+35.4853,2461171.8407,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.1949+35.4853 20260511.3407 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 11.3407 2461171.8407 11.46 22:12:11.79 +41:08:45.6
93.35103 -12.40333 galactic Lac Second-epoch detections are separated by 2.1" and 7.6 pix
The object was found in VSX15" Gaia DR3 1958027284753295360
Type: ROT
# Max. Min./Amp. JD0 Period
17.110 G 17.170 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:12:11.79 +41:08:45.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:12:11.79 +41:08:45.6: 13.76 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958027284753295360,2461171.8407,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958027284753295360 20260511.3407 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 11.3407 2461171.8407 11.55 21:43:17.64 +38:29:47.6
87.23804 -11.00459 galactic Cyg 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 J325.8236+38.4970 | 21:43:17.64 +38:29:47.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.680+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:17.64 +38:29:47.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:17.64 +38:29:47.6: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8236+38.4970,2461171.8407,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8236+38.4970 20260511.3407 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 11.3407 2461171.8407 11.47 21:40:43.77 +37:22:59.4
86.09643 -11.49613 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 J325.1759+37.3947 | 21:40:43.77 +37:22:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.217+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:43.77 +37:22:59.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:43.77 +37:22:59.4: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1759+37.3947,2461171.8407,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1759+37.3947 20260511.3407 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 11.3407 2461171.8407 11.46 21:27:41.84 +38:45:45.6
85.15973 -8.73396 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 J321.9265+38.7675 | 21:27:41.84 +38:45:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.638+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:41.84 +38:45:45.6: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:41.84 +38:45:45.6: 13.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 J321.9265+38.7675,2461171.8407,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.9265+38.7675 20260511.3407 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 11.3407 2461171.8407 11.62 21:36:54.33 +40:36:46.8
87.74765 -8.60813 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 J324.2332+40.6116 | 21:36:54.33 +40:36:46.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.644+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:54.33 +40:36:46.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:54.33 +40:36:46.8: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2332+40.6116,2461171.8407,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2332+40.6116 20260511.3407 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 11.3407 2461171.8407 11.60 21:59:40.16 +41:01:39.7
91.35126 -11.07972 galactic Lac Second-epoch detections are separated by 4.2" 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 J329.9159+41.0218 | 21:59:39.84 +41:01:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:40.16 +41:01:39.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:40.16 +41:01:39.7: 13.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9159+41.0218,2461171.8407,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9159+41.0218 20260511.3407 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 11.3407 2461171.8407 11.51 22:00:33.53 +41:25:45.6
91.73756 -10.86650 galactic Lac Second-epoch detections are separated by 6.2" 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 J330.1366+41.4294 | 22:00:33.53 +41:25:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.463+/-0.085 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:33.53 +41:25:45.6: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:33.53 +41:25:45.6: 13.62 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.1366+41.4294,2461171.8407,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.1366+41.4294 20260511.3407 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 11.3407 2461171.8407 11.39 22:01:22.50 +40:55:08.0
91.54162 -11.36367 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 | ATO J330.3389+40.9153 | 22:01:22.50 +40:55:08.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.776+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:22.50 +40:55:08.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:22.50 +40:55:08.0: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3389+40.9153,2461171.8407,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.3389+40.9153 20260511.3407 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 11.3407 2461171.8407 11.40 21:57:03.95 +40:57:15.4
90.91270 -10.83199 galactic Cyg Second-epoch detections are separated by 4.9" 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 | 21:57:03.95 +40:57:15.4 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:03.95 +40:57:15.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:03.95 +40:57:15.4: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.64 21:29:00.32 +38:59:30.9
85.50607 -8.74725 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 | Large-amplitude variable Gaia DR2 1964564358128327936 | 21:29:00.32 +38:59:30.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.358+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:00.32 +38:59:30.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:00.32 +38:59:30.9: 13.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1964564358128327936,2461171.8407,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1964564358128327936 20260511.3407 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 11.3407 2461171.8407 11.54 21:26:09.27 +40:15:20.0
86.00043 -7.45940 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 | ASASSN-V J212609.84+401448.8 | 21:26:10.64 +40:15:05.6 (Gaia DR3) | ROT: (local) | d (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:09.27 +40:15:20.0: 11.58 +/- 0.07 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:09.27 +40:15:20.0: 13.22 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
ASASSN-V J212609.84+401448.8,2461171.8407,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212609.84+401448.8 20260511.3407 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 11.3407 2461171.8407 11.41 21:32:29.76 +41:05:24.6
87.45835 -7.69110 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 | target | 21:32:29.76 +41:05:24.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.440+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:29.76 +41:05:24.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:29.76 +41:05:24.6: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.27 21:48:47.08 +40:08:12.7
89.14859 -10.46184 galactic Cyg Second-epoch detections are separated by 0.2" 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 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-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:47.08 +40:08:12.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:47.08 +40:08:12.7: 13.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 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+40.1375,2461171.8407,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1964+40.1375 20260511.3407 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 11.3407 2461171.8407 11.24 22:02:11.34 +35:32:41.3
88.25634 -15.68911 galactic Peg Second-epoch detections are separated by 1.8" 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 | Gaia DR3 1948505887717109376 | 22:02:11.25 +35:33:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:11.34 +35:32:41.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:11.34 +35:32:41.3: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1948505887717109376,2461171.8407,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1948505887717109376 20260511.3407 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 11.3407 2461171.8407 11.44 21:34:56.24 +40:57:06.9
87.70286 -8.10642 galactic Cyg Second-epoch detections are separated by 4.4" and 7.4 pix
The object was found in VSX 3" Gaia DR3 1966286850464992640
Type: ROT
# Max. Min./Amp. JD0 Period
14.110 G 14.130 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:56.24 +40:57:06.9: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:56.24 +40:57:06.9: 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 1966286850464992640,2461171.8407,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966286850464992640 20260511.3407 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 11.19 21:35:35.31 +35:59:25.8
84.35848 -11.81938 galactic Cyg Second-epoch detections are separated by 0.7" 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 | Gaia DR3 1951030748672306944 | 21:35:37.59 +35:59:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.355+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:35.31 +35:59:25.8: 12.91 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:35.31 +35:59:25.8: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951030748672306944,2461171.8407,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951030748672306944 20260511.3407 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 11.3407 2461171.8407 11.20 21:40:56.30 +41:13:23.8
88.73324 -8.66596 galactic Cyg Second-epoch detections are separated by 0.9" 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 J325.2343+41.2229 | 21:40:56.30 +41:13:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.331+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:56.30 +41:13:23.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:56.30 +41:13:23.8: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2343+41.2229,2461171.8407,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2343+41.2229 20260511.3407 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 11.3407 2461171.8407 11.12 21:32:44.34 +41:15:17.7
87.60582 -7.60237 galactic Cyg Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX20" NSV 25667
Type: LB
# Max. Min./Amp. JD0 Period
15.500 B 16.300 B C
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:44.34 +41:15:17.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:44.34 +41:15:17.7: 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
NSV 25667,2461171.8407,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 25667 20260511.3407 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 11.3407 2461171.8407 11.06 21:27:24.13 +33:39:56.9
81.46979 -12.31518 galactic Cyg Second-epoch detections are separated by 2.1" 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 | Gaia DR3 1854304305596960256 | 21:27:21.99 +33:40:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.028 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:24.13 +33:39:56.9: 11.36 +/- 0.06 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:24.13 +33:39:56.9: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 1854304305596960256,2461171.8407,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1854304305596960256 20260511.3407 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 11.3407 2461171.8407 10.81 22:05:39.73 +34:53:38.4
88.41751 -16.63924 galactic Peg Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX20" Gaia DR3 1900468744392395008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.160 G 13.190 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:39.73 +34:53:38.4: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:39.73 +34:53:38.4: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1900468744392395008,2461171.8407,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1900468744392395008 20260511.3407 10.81CV 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 11.3407 2461171.8407 11.01 21:35:27.08 +41:28:51.2
88.13708 -7.78361 galactic Cyg Second-epoch detections are separated by 1.6" 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 J323.8720+41.4829 | 21:35:28.88 +41:28:44.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.689+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:27.08 +41:28:51.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:27.08 +41:28:51.2: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8720+41.4829,2461171.8407,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8720+41.4829 20260511.3407 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 11.3407 2461171.8407 10.88 21:44:09.48 +37:55:02.4
86.97607 -11.55076 galactic Cyg Second-epoch detections are separated by 1.5" 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 J326.0405+37.9120 | 21:44:11.54 +37:55:07.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.406+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:09.48 +37:55:02.4: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:09.48 +37:55:02.4: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 J326.0405+37.9120,2461171.8407,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.0405+37.9120 20260511.3407 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 11.3407 2461171.8407 10.79 21:33:13.79 +37:12:42.6
84.86391 -10.60697 galactic Cyg Second-epoch detections are separated by 0.8" 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 | Gaia DR3 1952077135843691520 | 21:33:13.84 +37:13:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.344+/-0.031 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:13.79 +37:12:42.6: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:13.79 +37:12:42.6: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 1952077135843691520,2461171.8407,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952077135843691520 20260511.3407 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 10.80 21:31:02.18 +37:39:41.2
84.85992 -9.98109 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 | ATO J322.7506+37.6620 | 21:31:00.15 +37:39:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.033 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:02.18 +37:39:41.2: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:02.18 +37:39:41.2: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7506+37.6620,2461171.8407,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7506+37.6620 20260511.3407 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 10.70 21:37:46.82 +36:44:34.6
85.21230 -11.57077 galactic Cyg Second-epoch detections are separated by 1.2" and 7.1 pix
The object was found in VSX23" ASASSN-V J213745.82+364414.6
Type: L
# Max. Min./Amp. JD0 Period
11.610 V 11.730 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:46.82 +36:44:34.6: 13.27 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:46.82 +36:44:34.6: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213745.82+364414.6,2461171.8407,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213745.82+364414.6 20260511.3407 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 10.62 21:32:51.79 +35:15:26.5
83.43195 -11.96843 galactic Cyg 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 J323.2165+35.2577 | 21:32:51.79 +35:15:26.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.421+/-0.025 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:51.79 +35:15:26.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:51.79 +35:15:26.5: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.2165+35.2577,2461171.8407,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.2165+35.2577 20260511.3407 10.62CV 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 11.3407 2461171.8407 10.46 22:06:01.50 +39:10:17.5
91.17535 -13.29163 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 | 22:06:01.50 +39:10:17.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:06:01.50 +39:10:17.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:06:01.50 +39:10:17.5: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 10.46CV 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 11.3407 2461171.8407 10.62 21:28:09.36 +41:14:35.7
86.96895 -7.01657 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 J322.0200+41.2443 | 21:28:07.89 +41:14:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.370+/-0.033 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:09.36 +41:14:35.7: 12.25 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:09.36 +41:14:35.7: 12.32 +/- 0.02 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
ATO J322.0200+41.2443,2461171.8407,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0200+41.2443 20260511.3407 10.62CV 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 11.3407 2461171.8407 10.41 21:30:32.09 +35:46:45.3
83.45484 -11.26393 galactic Cyg 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 | 21:30:32.09 +35:46:45.3 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:32.09 +35:46:45.3: 12.75 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:32.09 +35:46:45.3: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 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,2461171.8407,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 10.41CV 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 11.3407 2461171.8407 10.19 22:01:26.27 +38:07:01.4
89.78381 -13.57840 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 | 22:01:26.27 +38:07:01.4 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:26.27 +38:07:01.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:26.27 +38:07:01.4: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 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,2461171.8407,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 9.91 21:59:06.42 +34:00:16.6
86.73690 -16.48997 galactic Peg Second-epoch detections are separated by 1.6" 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 | Gaia DR3 1947975824331378048 | 21:59:07.15 +34:00:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:06.42 +34:00:16.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:06.42 +34:00:16.6: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947975824331378048,2461171.8407,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947975824331378048 20260511.3407 9.91CV 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 11.3407 2461171.8407 10.12 21:36:49.73 +39:45:20.4
87.14990 -9.22983 galactic Cyg Second-epoch detections are separated by 0.8" 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 1965969366481229952 | 21:36:48.10 +39:45:16.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.284+/-0.035 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:49.73 +39:45:20.4: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:49.73 +39:45:20.4: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965969366481229952,2461171.8407,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965969366481229952 20260511.3407 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 11.3407 2461171.8407 9.65 21:34:29.38 +39:23:39.0
86.56605 -9.18847 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 | Gaia DR3 1965875770554661504 | 21:34:28.39 +39:23:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.762+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:29.38 +39:23:39.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:29.38 +39:23:39.0: 11.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965875770554661504,2461171.8407,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965875770554661504 20260511.3407 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 11.3407 2461171.8407 10.29 22:09:13.51 +39:15:45.3
91.74145 -13.59052 galactic Lac Second-epoch detections are separated by 0.5" 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 | Gaia DR3 1956289747146754688 | 22:09:11.61 +39:15:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.504+/-0.027 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:09:13.51 +39:15:45.3: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:09:13.51 +39:15:45.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 1956289747146754688,2461171.8407,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956289747146754688 20260511.3407 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 11.3407 2461171.8407 10.55 21:27:30.60 +37:13:07.7
84.03737 -9.81003 galactic Cyg Second-epoch detections are separated by 0.6" 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 J321.8820+37.2201 | 21:27:31.67 +37:13:36.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.725+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:30.60 +37:13:07.7: 12.57 +/- 0.17 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:30.60 +37:13:07.7: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 J321.8820+37.2201,2461171.8407,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8820+37.2201 20260511.3407 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 11.3407 2461171.8407 10.94 21:42:12.49 +38:54:22.8
87.35404 -10.55758 galactic Cyg Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX 4" ZTF J214212.23+385425.2
Type: RS:
# Max. Min./Amp. JD0 Period
13.756 r Y 0.081 r 2458607.86350 0.150071000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:12.49 +38:54:22.8: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:12.49 +38:54:22.8: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 J214212.23+385425.2,2461171.8407,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214212.23+385425.2 20260511.3407 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 11.3407 2461171.8407 11.06 21:44:26.41 +41:28:26.4
89.40008 -8.91191 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 | Gaia DR3 1954551797221475456 | 21:44:29.47 +41:28:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:26.41 +41:28:26.4: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:26.41 +41:28:26.4: 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
Gaia DR3 1954551797221475456,2461171.8407,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954551797221475456 20260511.3407 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 11.3407 2461171.8407 11.38 21:39:00.52 +38:41:35.3
86.73804 -10.29868 galactic Cyg Second-epoch detections are separated by 6.7" 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 J324.7488+38.6969 | 21:38:58.77 +38:41:57.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.697+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:00.52 +38:41:35.3: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:00.52 +38:41:35.3: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.7488+38.6969,2461171.8407,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7488+38.6969 20260511.3407 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 11.3407 2461171.8407 11.43 21:33:58.53 +36:17:17.2
84.32586 -11.37937 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ASASSN-V J213356.94+361650.1 | 21:33:56.95 +36:16:50.1 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:58.53 +36:17:17.2: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:58.53 +36:17:17.2: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213356.94+361650.1,2461171.8407,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213356.94+361650.1 20260511.3407 11.43CV 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 11.3407 2461171.8407 11.28 22:02:42.57 +41:44:10.0
92.25261 -10.86981 galactic Lac Second-epoch detections are separated by 0.8" 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 1959859277284333312 | 22:02:40.01 +41:44:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:42.57 +41:44:10.0: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:42.57 +41:44:10.0: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959859277284333312,2461171.8407,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959859277284333312 20260511.3407 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 11.3407 2461171.8407 11.36 21:54:02.63 +41:59:37.9
91.12839 -9.66748 galactic Cyg Second-epoch detections are separated by 0.8" 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 | Gaia DR3 1960440850219332992 | 21:54:04.11 +41:59:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.434+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:02.63 +41:59:37.9: 13.57 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:02.63 +41:59:37.9: 13.62 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 1960440850219332992,2461171.8407,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960440850219332992 20260511.3407 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 11.3407 2461171.8407 11.51 21:57:59.28 +41:37:11.8
91.47255 -10.41926 galactic Lac 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 | Gaia DR3 1959984174936797696 | 21:57:55.98 +41:36:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:59.28 +41:37:11.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:59.28 +41:37:11.8: 14.01 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959984174936797696,2461171.8407,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959984174936797696 20260511.3407 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 11.3407 2461171.8407 11.51 21:43:12.09 +34:12:51.4
84.29423 -14.18053 galactic Cyg 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 J325.7981+34.2157 | 21:43:11.59 +34:12:11.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:12.09 +34:12:51.4: 12.99 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:12.09 +34:12:51.4: 13.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 J325.7981+34.2157,2461171.8407,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7981+34.2157 20260511.3407 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 11.3407 2461171.8407 11.55 21:48:12.49 +41:41:11.4
90.08167 -9.20962 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 | Gaia DR3 1960503900338500992 | 21:48:14.24 +41:40:60.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.489+/-0.045 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:12.49 +41:41:11.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:12.49 +41:41:11.4: 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
Gaia DR3 1960503900338500992,2461171.8407,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960503900338500992 20260511.3407 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 11.3407 2461171.8407 11.65 21:29:54.96 +37:14:44.7
84.40418 -10.12556 galactic Cyg Second-epoch detections are separated by 4.5" 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 J322.4632+37.2562 | 21:29:53.76 +37:15:13.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:54.96 +37:14:44.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:54.96 +37:14:44.7: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.4632+37.2562,2461171.8407,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.4632+37.2562 20260511.3407 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 11.3407 2461171.8407 11.66 21:28:25.43 +36:06:45.9
83.38142 -10.72674 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 | 21:28:25.43 +36:06:45.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:25.43 +36:06:45.9: 12.92 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:25.43 +36:06:45.9: 14.09 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461171.8407,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.68 21:36:48.46 +38:51:41.2
86.53242 -9.88473 galactic Cyg Second-epoch detections are separated by 5.4" 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 J324.1997+38.8630 | 21:36:48.46 +38:51:41.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:48.46 +38:51:41.2: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:48.46 +38:51:41.2: 13.13 +/- 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
ATO J324.1997+38.8630,2461171.8407,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.1997+38.8630 20260511.3407 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 11.3407 2461171.8407 11.72 21:33:14.96 +33:54:30.5
82.53157 -12.99460 galactic Cyg Second-epoch detections are separated by 1.5" 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 | ASASSN-V J213311.49+335442.1 | 21:33:11.49 +33:54:42.1 (Gaia DR3) | SRS (local) | 22.560000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:14.96 +33:54:30.5: 12.59 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:14.96 +33:54:30.5: 14.06 +/- 0.11 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
ASASSN-V J213311.49+335442.1,2461171.8407,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213311.49+335442.1 20260511.3407 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 11.3407 2461171.8407 11.77 21:35:57.88 +41:51:55.4
88.47094 -7.56555 galactic Cyg Second-epoch detections are separated by 0.6" and 6.9 pix
The object was found in VSX14" Gaia DR3 1966751669007044992
Type: ROT
# Max. Min./Amp. JD0 Period
14.850 G 14.880 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:57.88 +41:51:55.4: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:57.88 +41:51:55.4: 13.83 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 1966751669007044992,2461171.8407,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966751669007044992 20260511.3407 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 11.3407 2461171.8407 11.68 21:27:38.07 +38:16:30.6
84.80566 -9.07374 galactic Cyg 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 | Gaia DR3 1964258114074497920 | 21:27:39.42 +38:15:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:38.07 +38:16:30.6: 11.91 +/- 0.09 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:38.07 +38:16:30.6: 13.80 +/- 0.09 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 1964258114074497920,2461171.8407,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964258114074497920 20260511.3407 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 11.3407 2461171.8407 11.56 22:10:19.98 +38:44:20.3
91.59922 -14.13954 galactic Lac Second-epoch detections are separated by 3.8" and 7.5 pix
The object was found in VSX 3" Gaia DR3 1955512632942240128
Type: ROT
# Max. Min./Amp. JD0 Period
13.880 G 13.920 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:10:19.98 +38:44:20.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:10:19.98 +38:44:20.3: 14.30 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1955512632942240128,2461171.8407,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955512632942240128 20260511.3407 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 11.3407 2461171.8407 11.71 21:34:43.04 +37:25:55.5
85.23650 -10.65019 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 1952179154205953792 | 21:34:40.19 +37:26:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:43.04 +37:25:55.5: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:43.04 +37:25:55.5: 14.04 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952179154205953792,2461171.8407,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952179154205953792 20260511.3407 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 11.3407 2461171.8407 11.85 21:26:46.15 +37:00:06.3
83.77591 -9.86067 galactic Cyg 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 | Gaia DR3 1963751960767702144 | 21:26:43.72 +36:59:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.428+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:46.15 +37:00:06.3: 13.08 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:46.15 +37:00:06.3: 14.23 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1963751960767702144,2461171.8407,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963751960767702144 20260511.3407 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 11.3407 2461171.8407 11.57 22:05:01.96 +41:27:43.6
92.43572 -11.35088 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 +41:27:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.327+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:05:01.96 +41:27:43.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:05:01.96 +41:27:43.6: 14.01 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.2733+41.4646,2461171.8407,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2733+41.4646 20260511.3407 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 11.3407 2461171.8407 11.94 21:27:39.75 +41:28:18.2
87.06200 -6.78801 galactic Cyg Second-epoch detections are separated by 3.2" 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 J321.9194+41.4735 | 21:27:39.75 +41:28:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:39.75 +41:28:18.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:39.75 +41:28:18.2: 14.16 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.9194+41.4735,2461171.8407,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.9194+41.4735 20260511.3407 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 11.3407 2461171.8407 11.90 21:37:13.68 +40:19:25.2
87.59572 -8.86293 galactic Cyg 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 | Gaia DR3 1966021868162235520 | 21:37:16.80 +40:18:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:13.68 +40:19:25.2: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:13.68 +40:19:25.2: 14.34 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1966021868162235520,2461171.8407,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1966021868162235520 20260511.3407 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 11.3407 2461171.8407 11.94 21:26:55.28 +38:03:54.4
84.55530 -9.12533 galactic Cyg 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 | Large-amplitude variable Gaia DR2 1964230213966061824 | 21:26:54.89 +38:03:17.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.835+/-0.029 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:55.28 +38:03:54.4: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:55.28 +38:03:54.4: 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
Large-amplitude variable Gaia DR2 1964230213966061824,2461171.8407,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1964230213966061824 20260511.3407 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 11.3407 2461171.8407 11.66 21:49:15.18 +35:18:20.3
86.00023 -14.18913 galactic Cyg 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 | 21:49:15.18 +35:18:20.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:15.18 +35:18:20.3: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:15.18 +35:18:20.3: 14.48 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.69 21:59:01.85 +36:26:57.2
88.32583 -14.58391 galactic Peg Second-epoch detections are separated by 1.9" 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 1949636430486534272 | 21:59:02.65 +36:26:18.3 (Gaia DR3) | VAR (local) | F (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:01.85 +36:26:57.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:01.85 +36:26:57.2: 13.74 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 1949636430486534272,2461171.8407,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949636430486534272 20260511.3407 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 11.3407 2461171.8407 12.00 21:27:12.39 +39:44:02.8
85.77741 -7.97287 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 | 21:27:12.39 +39:44:02.8 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:12.39 +39:44:02.8: 12.80 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:12.39 +39:44:02.8: 14.34 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461171.8407,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.98 21:29:34.38 +38:30:18.3
85.24374 -9.17400 galactic Cyg Second-epoch detections are separated by 2.1" 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 | ATO J322.3953+38.5053 | 21:29:34.38 +38:30:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.706+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:34.38 +38:30:18.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:34.38 +38:30:18.3: 14.31 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.3953+38.5053,2461171.8407,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.3953+38.5053 20260511.3407 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 11.3407 2461171.8407 11.56 22:02:04.57 +37:45:26.7
89.65682 -13.93891 galactic Lac Second-epoch detections are separated by 2.1" 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 | 22:02:04.57 +37:45:26.7 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.038 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:04.57 +37:45:26.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:04.57 +37:45:26.7: 14.37 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.37 +/- 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,2461171.8407,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.89 21:28:53.79 +35:00:37.1
82.66248 -11.57944 galactic Cyg Second-epoch detections are separated by 0.7" 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 | target | 21:28:53.79 +35:00:37.1 (user input) | T | P | (position from user input) J-Ks=0.588+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:53.79 +35:00:37.1: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:53.79 +35:00:37.1: 14.86 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.86 +/- 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,2461171.8407,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.83 21:56:00.57 +37:10:55.4
88.31948 -13.63383 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 21:56:00.57 +37:10:55.4 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:00.57 +37:10:55.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:00.57 +37:10:55.4: 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,2461171.8407,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.74 21:29:32.76 +34:41:59.4
82.53682 -11.89410 galactic Cyg Second-epoch detections are separated by 2.7" 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 J322.3922+34.7057 | 21:29:32.76 +34:41:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.543+/-0.060 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:32.76 +34:41:59.4: 12.57 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:32.76 +34:41:59.4: 13.98 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 J322.3922+34.7057,2461171.8407,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.3922+34.7057 20260511.3407 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 11.3407 2461171.8407 11.54 22:07:43.39 +37:37:05.2
90.48254 -14.73106 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 | ATO J331.9384+37.6117 | 22:07:43.39 +37:37:05.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:07:43.39 +37:37:05.2: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:07:43.39 +37:37:05.2: 14.14 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.9384+37.6117,2461171.8407,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.9384+37.6117 20260511.3407 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 11.3407 2461171.8407 11.95 21:29:00.60 +35:14:16.8
82.84248 -11.43358 galactic Cyg Second-epoch detections are separated by 6.8" 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 | 21:29:00.60 +35:14:16.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:00.60 +35:14:16.8: 12.86 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:00.60 +35:14:16.8: 14.34 +/- 0.14 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
target,2461171.8407,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.76 21:56:34.42 +37:00:26.7
88.29507 -13.84021 galactic Cyg 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 | 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-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:34.42 +37:00:26.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:34.42 +37:00:26.7: 14.31 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1949631375305780480,2461171.8407,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1949631375305780480 20260511.3407 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 11.3407 2461171.8407 11.99 21:36:18.34 +40:03:06.5
87.27827 -8.94401 galactic Cyg Second-epoch detections are separated by 2.3" 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 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-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:18.34 +40:03:06.5: 13.17 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:18.34 +40:03:06.5: 14.13 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.02 +/- 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+40.0481,2461171.8407,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0798+40.0481 20260511.3407 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 11.3407 2461171.8407 12.02 21:35:21.77 +41:16:18.0
87.98154 -7.92612 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 J323.8437+41.2602 | 21:35:21.77 +41:16:18.0 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.387+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:21.77 +41:16:18.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:21.77 +41:16:18.0: 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 J323.8437+41.2602,2461171.8407,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8437+41.2602 20260511.3407 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 11.3407 2461171.8407 11.82 21:30:44.48 +35:40:18.1
83.40898 -11.37025 galactic Cyg Second-epoch detections are separated by 1.9" 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 J322.6833+35.6739 | 21:30:44.48 +35:40:18.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:44.48 +35:40:18.1: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:44.48 +35:40:18.1: 13.99 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.99 +/- 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 J322.6833+35.6739,2461171.8407,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.6833+35.6739 20260511.3407 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 11.3407 2461171.8407 11.76 21:48:08.00 +39:26:18.2
88.59059 -10.91224 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 J327.0163+39.4455 | 21:48:06.78 +39:26:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:08.00 +39:26:18.2: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:08.00 +39:26:18.2: 13.79 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.0163+39.4455,2461171.8407,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.0163+39.4455 20260511.3407 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 11.3407 2461171.8407 12.05 21:28:41.27 +40:32:26.6
86.54965 -7.59162 galactic Cyg Second-epoch detections are separated by 3.3" 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 J322.1738+40.5403 | 21:28:41.27 +40:32:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:41.27 +40:32:26.6: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:41.27 +40:32:26.6: 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
ATO J322.1738+40.5403,2461171.8407,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.1738+40.5403 20260511.3407 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 11.3407 2461171.8407 12.06 21:26:43.80 +36:22:02.7
83.31654 -10.30551 galactic Cyg Second-epoch detections are separated by 7.4" and 9.0 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 | 21:26:43.80 +36:22:02.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:43.80 +36:22:02.7: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:43.80 +36:22:02.7: 14.32 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.32 +/- 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,2461171.8407,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.99 21:28:38.45 +34:34:49.6
82.31573 -11.84824 galactic Cyg Second-epoch detections are separated by 3.0" 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 | 21:28:38.45 +34:34:49.6 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:38.45 +34:34:49.6: 12.96 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:38.45 +34:34:49.6: 14.62 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461171.8407,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 11.87 21:50:34.29 +37:11:01.8
87.46679 -12.93779 galactic Cyg Second-epoch detections are separated by 2.1" 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 | 21:50:34.29 +37:11:01.8 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:34.29 +37:11:01.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:34.29 +37:11:01.8: 14.50 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.11 21:47:02.39 +41:50:19.7
90.01351 -8.95245 galactic Cyg Second-epoch detections are separated by 0.9" and 7.2 pix
The object was found in VSX 3" ZTF J214702.30+415021.9
Type: EW
# Max. Min./Amp. JD0 Period
15.395 g Y 0.536 g 2458372.77990 0.329482000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:02.39 +41:50:19.7: 12.34 +/- 0.14 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:02.39 +41:50:19.7: 14.64 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
ZTF J214702.30+415021.9,2461171.8407,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214702.30+415021.9 20260511.3407 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 11.3407 2461171.8407 11.82 21:30:51.93 +34:46:06.8
82.78388 -12.03480 galactic Cyg Second-epoch detections are separated by 2.4" 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 J322.7141+34.7705 | 21:30:51.93 +34:46:06.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:51.93 +34:46:06.8: 13.12 +/- 0.28 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:51.93 +34:46:06.8: 14.34 +/- 0.15 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 J322.7141+34.7705,2461171.8407,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7141+34.7705 20260511.3407 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 11.3407 2461171.8407 11.85 21:30:59.29 +35:39:20.0
83.43419 -11.41676 galactic Cyg Second-epoch detections are separated by 5.5" 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 J322.7458+35.6560 | 21:30:59.29 +35:39:20.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:59.29 +35:39:20.0: 13.01 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:59.29 +35:39:20.0: 14.55 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 J322.7458+35.6560,2461171.8407,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7458+35.6560 20260511.3407 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 11.3407 2461171.8407 11.98 21:28:05.38 +38:26:58.6
84.99376 -9.01144 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 | 21:28:05.38 +38:26:58.6 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:05.38 +38:26:58.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:05.38 +38:26:58.6: 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,2461171.8407,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.09 21:32:15.23 +37:15:00.3
84.74776 -10.44522 galactic Cyg Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 2" Gaia DR3 1952091777392161024
Type: ROT
# Max. Min./Amp. JD0 Period
14.590 G 14.620 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:15.23 +37:15:00.3: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:15.23 +37:15:00.3: 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
Gaia DR3 1952091777392161024,2461171.8407,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952091777392161024 20260511.3407 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 11.3407 2461171.8407 12.15 21:29:37.20 +34:35:10.6
82.46648 -11.98570 galactic Cyg Second-epoch detections are separated by 2.8" and 7.8 pix
The object was found in VSX 1" Gaia DR3 1950469035671582336
Type: ROT
# Max. Min./Amp. JD0 Period
14.480 G 14.500 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:37.20 +34:35:10.6: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:37.20 +34:35:10.6: 14.81 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950469035671582336,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950469035671582336 20260511.3407 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 11.3407 2461171.8407 11.87 21:56:29.29 +36:52:34.7
88.19587 -13.93081 galactic Cyg Second-epoch detections are separated by 2.2" 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 J329.1195+36.8762 | 21:56:29.29 +36:52:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.385+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:29.29 +36:52:34.7: 12.17 +/- 0.08 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:29.29 +36:52:34.7: 14.27 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.1195+36.8762,2461171.8407,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.1195+36.8762 20260511.3407 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 11.3407 2461171.8407 11.97 21:42:31.34 +35:51:14.4
85.31996 -12.87153 galactic Cyg 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 | ATO J325.6327+35.8537 | 21:42:31.34 +35:51:14.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:31.34 +35:51:14.4: 13.38 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:31.34 +35:51:14.4: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.6327+35.8537,2461171.8407,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6327+35.8537 20260511.3407 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 11.3407 2461171.8407 12.15 21:27:07.54 +35:14:55.6
82.57147 -11.15517 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 | target | 21:27:07.54 +35:14:55.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:07.54 +35:14:55.6: 12.92 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:07.54 +35:14:55.6: 14.35 +/- 0.14 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,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.17 21:26:49.68 +38:35:30.6
84.91615 -8.73713 galactic Cyg Second-epoch detections are separated by 2.5" 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 | Large-amplitude variable Gaia DR2 1964456575923697664 | 21:26:49.68 +38:35:30.6 (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=0.729+/-0.029 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:49.68 +38:35:30.6: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:49.68 +38:35:30.6: 14.39 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.39 +/- 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
Large-amplitude variable Gaia DR2 1964456575923697664,2461171.8407,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1964456575923697664 20260511.3407 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 11.3407 2461171.8407 12.15 21:36:08.49 +35:55:08.0
84.39162 -11.94822 galactic Cyg Second-epoch detections are separated by 2.2" 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 | 21:36:08.49 +35:55:08.0 (user input) | T | P | (position from user input) J-Ks=0.537+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:08.49 +35:55:08.0: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:08.49 +35:55:08.0: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.08 21:32:35.85 +35:36:09.3
83.63662 -11.68211 galactic Cyg Second-epoch detections are separated by 4.1" 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 J323.1465+35.6027 | 21:32:35.85 +35:36:09.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.444+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:35.85 +35:36:09.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:35.85 +35:36:09.3: 14.76 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.1465+35.6027,2461171.8407,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.1465+35.6027 20260511.3407 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 11.3407 2461171.8407 12.15 21:39:31.97 +40:39:06.6
88.14739 -8.91455 galactic Cyg Second-epoch detections are separated by 1.6" 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 J324.8818+40.6426 | 21:39:31.97 +40:39:06.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:31.97 +40:39:06.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:31.97 +40:39:06.6: 14.34 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.8818+40.6426,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.8818+40.6426 20260511.3407 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 11.3407 2461171.8407 12.29 21:28:25.12 +39:09:59.0
85.54633 -8.54276 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 | 21:28:25.12 +39:09:59.0 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:25.12 +39:09:59.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:25.12 +39:09:59.0: 14.81 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.21 21:26:44.70 +36:58:52.9
83.75787 -9.87176 galactic Cyg 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 | Gaia DR3 1963751960767702144 | 21:26:43.72 +36:59:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.339+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:44.70 +36:58:52.9: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:44.70 +36:58:52.9: 14.96 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.96 +/- 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 1963751960767702144,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1963751960767702144 20260511.3407 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 11.3407 2461171.8407 11.89 21:57:22.92 +41:48:54.2
91.50589 -10.19614 galactic Cyg Second-epoch detections are separated by 1.5" 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 | target | 21:57:22.92 +41:48:54.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:22.92 +41:48:54.2: 12.38 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:22.92 +41:48:54.2: 14.22 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461171.8407,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.12 21:28:21.49 +39:21:51.2
85.67723 -8.39272 galactic Cyg Second-epoch detections are separated by 5.3" and 6.6 pix
The object was found in VSX 5" Gaia DR3 1964588379877968000
Type: ROT
# Max. Min./Amp. JD0 Period
14.690 G 14.720 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:21.49 +39:21:51.2: 13.12 +/- 0.25 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:21.49 +39:21:51.2: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.10 +/- 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 1964588379877968000,2461171.8407,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964588379877968000 20260511.3407 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 11.3407 2461171.8407 12.25 21:29:38.89 +36:14:26.1
83.65211 -10.80842 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 | target | 21:29:38.89 +36:14:26.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:38.89 +36:14:26.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:38.89 +36:14:26.1: 14.80 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.16 21:34:17.58 +36:20:30.7
84.41093 -11.38443 galactic Cyg Second-epoch detections are separated by 2.1" 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 | 21:34:17.58 +36:20:30.7 (user input) | T | P | (position from user input) J-Ks=0.245+/-0.046 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:17.58 +36:20:30.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:17.58 +36:20:30.7: 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,2461171.8407,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.15 21:28:43.67 +35:42:02.8
83.13179 -11.06352 galactic Cyg Second-epoch detections are separated by 3.7" 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 | 21:28:43.67 +35:42:02.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.67 +35:42:02.8: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.67 +35:42:02.8: 15.13 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.13 +/- 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,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.19 21:46:36.96 +37:07:18.4
86.81339 -12.47006 galactic Cyg 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 | Gaia DR3 1952535116796630656 | 21:46:38.74 +37:07:55.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=0.402+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:36.96 +37:07:18.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:36.96 +37:07:18.4: 14.81 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.81 +/- 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 1952535116796630656,2461171.8407,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952535116796630656 20260511.3407 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 11.3407 2461171.8407 12.13 21:40:15.11 +36:00:22.8
85.07640 -12.44964 galactic Cyg Second-epoch detections are separated by 1.9" 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 | 21:40:15.11 +36:00:22.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:15.11 +36:00:22.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:15.11 +36:00:22.8: 14.69 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.69 +/- 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,2461171.8407,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.04 21:32:09.67 +40:20:08.4
86.88904 -8.19645 galactic Cyg Second-epoch detections are separated by 4.4" 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 J323.0372+40.3368 | 21:32:09.67 +40:20:08.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:09.67 +40:20:08.4: 12.00 +/- 0.10 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:09.67 +40:20:08.4: 13.98 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 J323.0372+40.3368,2461171.8407,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.0372+40.3368 20260511.3407 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 11.3407 2461171.8407 12.21 21:33:29.39 +37:59:53.2
85.45189 -10.07189 galactic Cyg Second-epoch detections are separated by 1.6" and 7.3 pix
The object was found in VSX18" Gaia DR3 1952276632785584512
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.930 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:29.39 +37:59:53.2: 13.15 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:29.39 +37:59:53.2: 14.34 +/- 0.13 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
Gaia DR3 1952276632785584512,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952276632785584512 20260511.3407 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 11.3407 2461171.8407 11.98 21:31:50.24 +41:32:44.7
87.68268 -7.27471 galactic Cyg Second-epoch detections are separated by 5.8" 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 | Gaia DR3 1967127736343468288 | 21:31:53.89 +41:32:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:50.24 +41:32:44.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:50.24 +41:32:44.7: 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 1967127736343468288,2461171.8407,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967127736343468288 20260511.3407 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 11.3407 2461171.8407 12.17 22:02:09.53 +41:51:03.0
92.24090 -10.71630 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 | 22:02:09.53 +41:51:03.0 (user input) | T | P | (position from user input) J-Ks=0.676+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:09.53 +41:51:03.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:09.53 +41:51:03.0: 14.88 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.88 +/- 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,2461171.8407,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.15 21:51:39.08 +36:55:29.1
87.46332 -13.27473 galactic Cyg Second-epoch detections are separated by 2.1" 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 J327.8989+36.9256 | 21:51:39.08 +36:55:29.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.499+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.08 +36:55:29.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.08 +36:55:29.1: 15.46 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.46 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.8989+36.9256,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.8989+36.9256 20260511.3407 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 11.3407 2461171.8407 12.20 21:28:08.33 +36:20:38.4
83.50483 -10.52164 galactic Cyg 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 | ATO J322.0319+36.3316 | 21:28:08.33 +36:20:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:08.33 +36:20:38.4: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:08.33 +36:20:38.4: 14.85 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0319+36.3316,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0319+36.3316 20260511.3407 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 11.3407 2461171.8407 11.98 21:32:38.88 +34:43:57.6
83.02703 -12.31562 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 | target | 21:32:38.88 +34:43:57.6 (user input) | T | P | (position from user input) J-Ks=0.853+/-0.026 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:38.88 +34:43:57.6: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:38.88 +34:43:57.6: 14.28 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461171.8407,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.05 21:43:05.89 +37:32:43.5
86.56398 -11.68971 galactic Cyg 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 | target | 21:43:05.89 +37:32:43.5 (user input) | T | P | (position from user input) J-Ks=0.764+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:05.89 +37:32:43.5: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:05.89 +37:32:43.5: 14.79 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.79 +/- 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,2461171.8407,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.12 21:46:29.48 +40:15:30.5
88.89075 -10.08474 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 | target | 21:46:29.48 +40:15:30.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:29.48 +40:15:30.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:29.48 +40:15:30.5: 14.71 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.12 21:41:04.96 +34:50:45.4
84.40042 -13.41975 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 | Gaia DR3 1950661140965705344 | 21:41:05.70 +34:51:24.0 (Gaia DR3) | ROT (local) | K (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.458+/-0.060 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:04.96 +34:50:45.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:04.96 +34:50:45.4: 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
Gaia DR3 1950661140965705344,2461171.8407,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950661140965705344 20260511.3407 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 11.3407 2461171.8407 12.26 21:36:03.50 +41:27:53.0
88.21048 -7.87250 galactic Cyg Second-epoch detections are separated by 1.4" 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 | ATO J324.0074+41.4709 | 21:36:03.50 +41:27:53.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.455+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:03.50 +41:27:53.0: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:03.50 +41:27:53.0: 14.64 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.64 +/- 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 J324.0074+41.4709,2461171.8407,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0074+41.4709 20260511.3407 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 11.3407 2461171.8407 12.27 21:26:38.67 +38:32:27.5
84.85419 -8.74821 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 J321.6532+38.5492 | 21:26:38.67 +38:32:27.5 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:38.67 +38:32:27.5: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:38.67 +38:32:27.5: 14.96 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.96 +/- 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 J321.6532+38.5492,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.6532+38.5492 20260511.3407 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 11.3407 2461171.8407 12.32 21:27:19.93 +35:12:54.6
82.57776 -11.20874 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 | ATO J321.8331+35.2169 | 21:27:19.93 +35:12:54.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.439+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:19.93 +35:12:54.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:19.93 +35:12:54.6: 14.66 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.8331+35.2169,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.8331+35.2169 20260511.3407 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 11.3407 2461171.8407 12.12 21:36:10.81 +41:24:44.2
88.19165 -7.92658 galactic Cyg Second-epoch detections are separated by 0.6" 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 | ATO J324.0396+41.4060 | 21:36:10.81 +41:24:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:10.81 +41:24:44.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:10.81 +41:24:44.2: 14.70 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.0396+41.4060,2461171.8407,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0396+41.4060 20260511.3407 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 11.3407 2461171.8407 12.13 21:31:39.39 +36:46:27.4
84.32516 -10.70605 galactic Cyg Second-epoch detections are separated by 5.5" 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 | target | 21:31:39.39 +36:46:27.4 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:39.39 +36:46:27.4: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:39.39 +36:46:27.4: 14.48 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.31 21:27:17.19 +38:38:14.0
85.01298 -8.76751 galactic Cyg Second-epoch detections are separated by 2.1" 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 | 21:27:17.19 +38:38:14.0 (user input) | T | P | (position from user input) J-Ks=0.935+/-0.032 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:17.19 +38:38:14.0: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:17.19 +38:38:14.0: 14.80 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.80 +/- 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,2461171.8407,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.22 21:35:57.22 +40:17:36.8
87.39411 -8.72071 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 | ATO J323.9864+40.2940 | 21:35:57.22 +40:17:36.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.395+/-0.062 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:57.22 +40:17:36.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:57.22 +40:17:36.8: 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
ATO J323.9864+40.2940,2461171.8407,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.9864+40.2940 20260511.3407 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 11.3407 2461171.8407 12.49 21:28:47.59 +41:03:28.1
86.92614 -7.23330 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 | 21:28:47.59 +41:03:28.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:47.59 +41:03:28.1: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:47.59 +41:03:28.1: 14.80 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.26 21:32:33.19 +38:39:50.3
85.78128 -9.46219 galactic Cyg Second-epoch detections are separated by 0.6" 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 | 21:32:33.19 +38:39:50.3 (user input) | T | P | (position from user input) J-Ks=0.801+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:33.19 +38:39:50.3: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:33.19 +38:39:50.3: 14.76 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.13 21:44:32.22 +40:17:32.3
88.62736 -9.81494 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 | target | 21:44:32.22 +40:17:32.3 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.410+/-0.048 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:32.22 +40:17:32.3: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:32.22 +40:17:32.3: 14.93 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.93 +/- 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,2461171.8407,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.21 21:34:14.73 +36:36:51.4
84.59496 -11.18015 galactic Cyg Second-epoch detections are separated by 3.7" 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 | Gaia DR3 1951856168364151680 | 21:34:12.08 +36:37:06.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.747+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:14.73 +36:36:51.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:14.73 +36:36:51.4: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951856168364151680,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951856168364151680 20260511.3407 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 11.3407 2461171.8407 12.25 21:28:43.52 +36:04:03.0
83.39333 -10.80171 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 21:28:43.52 +36:04:03.0 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:43.52 +36:04:03.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:43.52 +36:04:03.0: 14.87 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.87 +/- 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,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.36 21:28:44.18 +38:13:29.3
84.92677 -9.26092 galactic Cyg Second-epoch detections are separated by 1.9" 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 | 21:28:44.18 +38:13:29.3 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:44.18 +38:13:29.3: 12.76 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:44.18 +38:13:29.3: 14.62 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.41 21:35:31.74 +40:47:48.9
87.67944 -8.29615 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 | ATO J323.8732+40.8073 | 21:35:31.74 +40:47:48.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:31.74 +40:47:48.9: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:31.74 +40:47:48.9: 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 J323.8732+40.8073,2461171.8407,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8732+40.8073 20260511.3407 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 11.3407 2461171.8407 12.21 21:31:57.29 +36:19:01.8
84.04638 -11.07699 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 21:31:57.29 +36:19:01.8 (user input) | T | P | (position from user input) J-Ks=0.708+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:57.29 +36:19:01.8: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:57.29 +36:19:01.8: 14.63 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.63 +/- 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,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.16 21:42:45.62 +38:41:53.6
87.29499 -10.78455 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 | 21:42:45.62 +38:41:53.6 (user input) | T | P | (position from user input) J-Ks=0.661+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:45.62 +38:41:53.6: 12.55 +/- 0.12 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:45.62 +38:41:53.6: 14.86 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461171.8407,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.03 21:42:33.69 +41:45:50.0
89.32575 -8.46256 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 | target | 21:42:33.69 +41:45:50.0 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:33.69 +41:45:50.0: 13.14 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:33.69 +41:45:50.0: 14.21 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.24 21:51:39.57 +40:18:34.1
89.68886 -10.68289 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 | target | 21:51:39.57 +40:18:34.1 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:39.57 +40:18:34.1: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:39.57 +40:18:34.1: 14.92 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.92 +/- 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,2461171.8407,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.14 21:35:10.37 +39:24:30.9
86.67379 -9.26794 galactic Cyg 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 | ATO J323.7976+39.3988 | 21:35:10.37 +39:24:30.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.686+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:10.37 +39:24:30.9: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:10.37 +39:24:30.9: 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 J323.7976+39.3988,2461171.8407,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.7976+39.3988 20260511.3407 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 11.3407 2461171.8407 12.17 21:28:40.93 +39:00:16.9
85.46947 -8.69436 galactic Cyg Second-epoch detections are separated by 2.4" 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 J322.1768+39.0006 | 21:28:40.93 +39:00:16.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:40.93 +39:00:16.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:40.93 +39:00:16.9: 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 J322.1768+39.0006,2461171.8407,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.1768+39.0006 20260511.3407 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 11.3407 2461171.8407 12.36 21:37:11.01 +41:54:60.0
88.67476 -7.68076 galactic Cyg Second-epoch detections are separated by 0.8" 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 J324.2958+41.9173 | 21:37:11.01 +41:54:60.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.754+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:11.01 +41:54:60.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:11.01 +41:54:60.0: 14.63 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2958+41.9173,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2958+41.9173 20260511.3407 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 11.3407 2461171.8407 12.34 21:31:07.07 +41:09:16.3
87.31264 -7.46605 galactic Cyg Second-epoch detections are separated by 1.6" 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 | 21:31:07.07 +41:09:16.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.765+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:07.07 +41:09:16.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:07.07 +41:09:16.3: 14.65 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.21 21:31:53.06 +36:06:56.4
83.89348 -11.21227 galactic Cyg Second-epoch detections are separated by 3.6" 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 | 21:31:53.06 +36:06:56.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:53.06 +36:06:56.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:53.06 +36:06:56.4: 14.71 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.71 +/- 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,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.14 21:50:31.71 +38:39:09.1
88.43272 -11.81217 galactic Cyg 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 | 21:50:31.71 +38:39:09.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.422+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:31.71 +38:39:09.1: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:31.71 +38:39:09.1: 14.73 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.73 +/- 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,2461171.8407,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.11 21:57:10.53 +42:10:40.2
91.70479 -9.88837 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 | 21:57:10.53 +42:10:40.2 (user input) | T | P | (position from user input) J-Ks=0.180+/-0.064 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:57:10.53 +42:10:40.2: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:57:10.53 +42:10:40.2: 14.30 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.26 21:46:56.37 +37:17:26.5
86.97681 -12.38512 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 | target | 21:46:56.37 +37:17:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:56.37 +37:17:26.5: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:56.37 +37:17:26.5: 15.32 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.32 +/- 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,2461171.8407,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.17 21:55:16.04 +41:56:18.7
91.27235 -9.85365 galactic Cyg Second-epoch detections are separated by 0.8" 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 | ATO J328.8166+41.9391 | 21:55:16.04 +41:56:18.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.675+/-0.046 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:16.04 +41:56:18.7: 13.27 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:16.04 +41:56:18.7: 14.26 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 J328.8166+41.9391,2461171.8407,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.8166+41.9391 20260511.3407 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 11.3407 2461171.8407 12.24 21:28:33.73 +35:11:45.3
82.74590 -11.39931 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 | ATO J322.1418+35.1952 | 21:28:33.73 +35:11:45.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:33.73 +35:11:45.3: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:33.73 +35:11:45.3: 14.96 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.96 +/- 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 J322.1418+35.1952,2461171.8407,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.1418+35.1952 20260511.3407 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 11.3407 2461171.8407 12.20 21:38:19.71 +39:47:35.3
87.39095 -9.39672 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 J324.5932+39.7857 | 21:38:19.71 +39:47:35.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.400+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:38:19.71 +39:47:35.3: 13.39 +/- 0.33 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:38:19.71 +39:47:35.3: 14.90 +/- 0.22 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
ATO J324.5932+39.7857,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.5932+39.7857 20260511.3407 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 11.3407 2461171.8407 12.43 21:31:41.34 +38:39:50.7
85.65748 -9.34583 galactic Cyg Second-epoch detections are separated by 2.0" 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 | target | 21:31:41.34 +38:39:50.7 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:41.34 +38:39:50.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:41.34 +38:39:50.7: 14.91 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.24 21:29:50.36 +34:12:18.7
82.22593 -12.28896 galactic Cyg 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 | target | 21:29:50.36 +34:12:18.7 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.030 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:50.36 +34:12:18.7: 13.02 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:50.36 +34:12:18.7: 14.81 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461171.8407,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.27 21:36:24.24 +40:56:09.1
87.89754 -8.30601 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 | ATO J324.0891+40.9406 | 21:36:24.24 +40:56:09.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.432+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:24.24 +40:56:09.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:24.24 +40:56:09.1: 14.75 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.75 +/- 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 J324.0891+40.9406,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0891+40.9406 20260511.3407 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 11.3407 2461171.8407 12.15 21:26:38.83 +39:47:21.9
85.73892 -7.85815 galactic Cyg 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 | 21:26:38.83 +39:47:21.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:38.83 +39:47:21.9: 13.07 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:38.83 +39:47:21.9: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461171.8407,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.21 21:26:51.58 +34:03:09.6
81.66872 -11.96230 galactic Cyg Second-epoch detections are separated by 2.7" and 7.3 pix
The object was found in VSX24" Gaia DR3 1855099733538948736
Type: ROT
# Max. Min./Amp. JD0 Period
16.960 G 17.080 G 0.491688000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:51.58 +34:03:09.6: 13.04 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:51.58 +34:03:09.6: 14.64 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855099733538948736,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1855099733538948736 20260511.3407 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 11.3407 2461171.8407 12.29 21:28:36.97 +36:44:01.2
83.85206 -10.31091 galactic Cyg Second-epoch detections are separated by 1.5" 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 | target | 21:28:36.97 +36:44:01.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:36.97 +36:44:01.2: 12.99 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:36.97 +36:44:01.2: 14.55 +/- 0.18 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
target,2461171.8407,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.29 21:32:17.26 +41:34:26.1
87.76397 -7.31198 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 | target | 21:32:17.26 +41:34:26.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:17.26 +41:34:26.1: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:17.26 +41:34:26.1: 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,2461171.8407,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.41 21:26:38.36 +41:30:09.8
86.94543 -6.63220 galactic Cyg Second-epoch detections are separated by 2.9" and 7.1 pix
The object was found in VSX 1" Gaia DR3 1967265037858771456
Type: ROT
# Max. Min./Amp. JD0 Period
14.610 G 14.640 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:38.36 +41:30:09.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:38.36 +41:30:09.8: 14.85 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.85 +/- 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 1967265037858771456,2461171.8407,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967265037858771456 20260511.3407 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 11.3407 2461171.8407 12.20 21:43:56.61 +39:49:06.2
88.22367 -10.09672 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 | 21:43:56.61 +39:49:06.2 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:56.61 +39:49:06.2: 13.13 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:56.61 +39:49:06.2: 14.51 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.35 21:28:20.86 +36:08:60.0
83.39687 -10.68941 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 | ATO J322.0938+36.1463 | 21:28:20.86 +36:08:60.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:20.86 +36:08:60.0: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:20.86 +36:08:60.0: 14.90 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.90 +/- 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 J322.0938+36.1463,2461171.8407,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0938+36.1463 20260511.3407 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 11.3407 2461171.8407 12.20 21:32:16.51 +41:10:13.7
87.48334 -7.60412 galactic Cyg Second-epoch detections are separated by 0.2" and 7.0 pix
The object was found in VSX11" 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-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:16.51 +41:10:13.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:16.51 +41:10:13.7: 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+411016.2,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213215.55+411016.2 20260511.3407 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 11.3407 2461171.8407 12.27 21:33:48.63 +40:09:52.7
87.00228 -8.53665 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 | target | 21:33:48.63 +40:09:52.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:48.63 +40:09:52.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:48.63 +40:09:52.7: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.25 21:29:41.64 +39:40:21.7
86.08117 -8.35006 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 | ATO J322.4137+39.6767 | 21:29:41.64 +39:40:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.720+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:41.64 +39:40:21.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:41.64 +39:40:21.7: 14.88 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.4137+39.6767,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.4137+39.6767 20260511.3407 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 11.3407 2461171.8407 12.11 21:33:24.18 +35:46:28.9
83.87880 -11.67111 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 21:33:24.18 +35:46:28.9 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.031 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:24.18 +35:46:28.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:24.18 +35:46:28.9: 15.03 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.03 +/- 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,2461171.8407,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.22 21:32:11.98 +41:33:25.9
87.74033 -7.31287 galactic Cyg Second-epoch detections are separated by 0.4" 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 | 21:32:11.98 +41:33:25.9 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:11.98 +41:33:25.9: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:11.98 +41:33:25.9: 14.56 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.32 21:28:45.01 +38:10:24.9
84.89253 -9.29952 galactic Cyg 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 | ATO J322.1854+38.1746 | 21:28:45.01 +38:10:24.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.064 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:45.01 +38:10:24.9: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:45.01 +38:10:24.9: 15.13 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.13 +/- 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 J322.1854+38.1746,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.1854+38.1746 20260511.3407 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 11.3407 2461171.8407 12.23 21:44:55.04 +40:18:07.5
88.68936 -9.85522 galactic Cyg 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 | 21:44:55.04 +40:18:07.5 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:55.04 +40:18:07.5: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:55.04 +40:18:07.5: 15.07 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.07 +/- 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,2461171.8407,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.35 21:28:24.59 +39:10:26.3
85.55043 -8.53613 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 | 21:28:24.59 +39:10:26.3 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:24.59 +39:10:26.3: 13.43 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:24.59 +39:10:26.3: 14.69 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461171.8407,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.26 21:32:20.07 +33:48:08.4
82.31583 -12.93858 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 | target | 21:32:20.07 +33:48:08.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:20.07 +33:48:08.4: 13.02 +/- 0.26 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:20.07 +33:48:08.4: 15.11 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461171.8407,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:30:16.06 +39:31:30.0
86.05826 -8.53312 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 J322.5811+39.5298 | 21:30:16.06 +39:31:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.438+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:16.06 +39:31:30.0: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:16.06 +39:31:30.0: 14.91 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.5811+39.5298,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.5811+39.5298 20260511.3407 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 11.3407 2461171.8407 12.30 21:31:06.96 +39:46:47.1
86.35561 -8.46190 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 | 21:31:06.96 +39:46:47.1 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.044 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:06.96 +39:46:47.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:06.96 +39:46:47.1: 14.75 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.75 +/- 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,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.30 21:28:27.96 +35:31:22.4
82.96591 -11.15286 galactic Cyg Second-epoch detections are separated by 2.1" 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 | Gaia DR3 1951320401268157696 | 21:28:25.92 +35:30:54.1 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:27.96 +35:31:22.4: 13.25 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:27.96 +35:31:22.4: 14.38 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1951320401268157696,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951320401268157696 20260511.3407 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 11.3407 2461171.8407 12.22 21:53:00.58 +35:46:12.7
86.91097 -14.33307 galactic Peg Second-epoch detections are separated by 1.5" 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 | target | 21:53:00.58 +35:46:12.7 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:00.58 +35:46:12.7: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:00.58 +35:46:12.7: 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,2461171.8407,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.32 21:34:31.85 +40:00:32.6
86.99669 -8.74439 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 | ATO J323.6318+40.0063 | 21:34:31.85 +40:00:32.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:31.85 +40:00:32.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:31.85 +40:00:32.6: 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 J323.6318+40.0063,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.6318+40.0063 20260511.3407 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 11.3407 2461171.8407 12.39 21:35:58.37 +39:59:36.1
87.19074 -8.94375 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 | 21:35:58.37 +39:59:36.1 (user input) | T | P | (position from user input) J-Ks=0.653+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:58.37 +39:59:36.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:58.37 +39:59:36.1: 15.08 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:45:57.17 +39:56:06.6
88.59684 -10.26206 galactic Cyg Second-epoch detections are separated by 2.3" 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 | 21:45:57.17 +39:56:06.6 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:57.17 +39:56:06.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:57.17 +39:56:06.6: 14.69 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.69 +/- 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,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.22 21:43:24.96 +38:44:40.6
87.42373 -10.83472 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 | ATO J325.8423+38.7409 | 21:43:24.96 +38:44:40.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.705+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:24.96 +38:44:40.6: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:24.96 +38:44:40.6: 14.92 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8423+38.7409,2461171.8407,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.8423+38.7409 20260511.3407 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 11.3407 2461171.8407 12.32 21:31:57.16 +41:47:00.4
87.86284 -7.11655 galactic Cyg Second-epoch detections are separated by 2.5" and 7.3 pix
The object was found in VSX 4" Gaia DR3 1967143335664994688
Type: ROT
# Max. Min./Amp. JD0 Period
15.120 G 15.150 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:57.16 +41:47:00.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:57.16 +41:47:00.4: 14.73 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.73 +/- 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 1967143335664994688,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967143335664994688 20260511.3407 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 11.3407 2461171.8407 12.28 21:32:40.29 +34:47:34.8
83.07348 -12.27557 galactic Cyg 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 | Large-amplitude variable Gaia DR2 1950555136871717632 | 21:32:40.29 +34:47:34.8 (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=0.746+/-0.025 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:40.29 +34:47:34.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:40.29 +34:47:34.8: 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
Large-amplitude variable Gaia DR2 1950555136871717632,2461171.8407,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1950555136871717632 20260511.3407 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 11.3407 2461171.8407 12.12 21:47:32.45 +41:45:09.2
90.02883 -9.07867 galactic Cyg Second-epoch detections are separated by 4.6" 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 J326.8748+41.7603 | 21:47:29.97 +41:45:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:32.45 +41:45:09.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:32.45 +41:45:09.2: 14.43 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.8748+41.7603,2461171.8407,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.8748+41.7603 20260511.3407 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 11.3407 2461171.8407 12.23 21:49:58.72 +41:45:12.8
90.38149 -9.37115 galactic Cyg Second-epoch detections are separated by 1.3" 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 J327.5029+41.7516 | 21:49:58.72 +41:45:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:58.72 +41:45:12.8: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:58.72 +41:45:12.8: 14.65 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.5029+41.7516,2461171.8407,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.5029+41.7516 20260511.3407 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 11.3407 2461171.8407 12.18 21:43:28.73 +37:46:48.3
86.78073 -11.56453 galactic Cyg Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX18" Gaia DR3 1952809964643278080
Type: RS
# Max. Min./Amp. JD0 Period
16.190 G 16.250 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:28.73 +37:46:48.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:28.73 +37:46:48.3: 14.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952809964643278080,2461171.8407,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952809964643278080 20260511.3407 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 11.3407 2461171.8407 12.28 21:41:24.07 +39:05:04.5
87.35589 -10.32019 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 21:41:24.07 +39:05:04.5 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:24.07 +39:05:04.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:24.07 +39:05:04.5: 15.12 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.08 21:37:25.90 +37:09:17.1
85.44562 -11.22131 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 | target | 21:37:25.90 +37:09:17.1 (user input) | T | P | (position from user input) J-Ks=0.745+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:25.90 +37:09:17.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:25.90 +37:09:17.1: 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
target,2461171.8407,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.13 21:54:32.74 +35:25:30.7
86.92851 -14.79808 galactic Peg Second-epoch detections are separated by 3.0" 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 | 21:54:32.74 +35:25:30.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:32.74 +35:25:30.7: 13.03 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:32.74 +35:25:30.7: 14.96 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.31 21:42:01.73 +41:13:56.3
88.89447 -8.79530 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 | 21:42:01.73 +41:13:56.3 (user input) | T | P | (position from user input) J-Ks=0.958+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:01.73 +41:13:56.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:01.73 +41:13:56.3: 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,2461171.8407,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.45 21:29:41.34 +41:08:36.9
87.10873 -7.28836 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 | target | 21:29:41.34 +41:08:36.9 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.048 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:41.34 +41:08:36.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:41.34 +41:08:36.9: 14.87 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.24 21:35:51.43 +40:29:40.1
87.51827 -8.56060 galactic Cyg Second-epoch detections are separated by 2.5" and 7.3 pix
The object was found in VSX12" NSV 13804
Type:
# Max. Min./Amp. JD0 Period
15.200 pg 16.200 pg
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:51.43 +40:29:40.1: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:51.43 +40:29:40.1: 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
NSV 13804,2461171.8407,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 13804 20260511.3407 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 11.3407 2461171.8407 12.32 21:48:42.14 +37:37:36.5
87.47280 -12.35988 galactic Cyg Second-epoch detections are separated by 1.3" and 7.4 pix
The object was found in VSX19" Gaia DR3 1952572779367739520
Type: ROT
# Max. Min./Amp. JD0 Period
16.870 G 16.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:42.14 +37:37:36.5: 13.24 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:42.14 +37:37:36.5: 14.96 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.30 +/- 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 1952572779367739520,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952572779367739520 20260511.3407 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 11.3407 2461171.8407 12.41 21:40:37.29 +42:07:42.5
89.29681 -7.95048 galactic Cyg 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 J325.1445+42.1225 | 21:40:37.29 +42:07:42.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:37.29 +42:07:42.5: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:37.29 +42:07:42.5: 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
ATO J325.1445+42.1225,2461171.8407,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1445+42.1225 20260511.3407 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 11.3407 2461171.8407 12.35 21:28:21.99 +40:06:48.3
86.20541 -7.85616 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 | 21:28:21.99 +40:06:48.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:21.99 +40:06:48.3: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:21.99 +40:06:48.3: 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,2461171.8407,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.27 21:36:17.98 +38:04:45.5
85.91846 -10.39105 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 | ATO J324.0741+38.0876 | 21:36:17.98 +38:04:45.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.582+/-0.042 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:17.98 +38:04:45.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:17.98 +38:04:45.5: 14.82 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.82 +/- 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 J324.0741+38.0876,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.0741+38.0876 20260511.3407 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 11.3407 2461171.8407 12.31 21:33:39.97 +33:37:45.1
82.39627 -13.25564 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 | target | 21:33:39.97 +33:37:45.1 (user input) | T | P | (position from user input) J-Ks=0.624+/-0.028 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:39.97 +33:37:45.1: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:39.97 +33:37:45.1: 14.92 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:51:40.04 +38:49:49.0
88.72324 -11.81916 galactic Cyg Second-epoch detections are separated by 3.0" 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 | target | 21:51:40.04 +38:49:49.0 (user input) | T | P | (position from user input) J-Ks=0.772+/-0.033 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:40.04 +38:49:49.0: 13.09 +/- 0.22 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:40.04 +38:49:49.0: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.25 21:46:24.78 +41:13:00.8
89.51354 -9.34855 galactic Cyg Second-epoch detections are separated by 5.1" and 7.2 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-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:24.78 +41:13:00.8: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:24.78 +41:13:00.8: 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
VARIABLE_NAME,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260511.3407 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 11.3407 2461171.8407 12.23 21:59:42.19 +41:00:47.0
91.34716 -11.09517 galactic Lac 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 J329.9159+41.0218 | 21:59:39.84 +41:01:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.038 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:42.19 +41:00:47.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:42.19 +41:00:47.0: 14.72 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9159+41.0218,2461171.8407,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9159+41.0218 20260511.3407 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 11.3407 2461171.8407 12.31 21:26:49.77 +40:01:27.0
85.92994 -7.71494 galactic Cyg Second-epoch detections are separated by 1.6" 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 J321.6974+40.0274 | 21:26:49.77 +40:01:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.330+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:49.77 +40:01:27.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:49.77 +40:01:27.0: 14.53 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.6974+40.0274,2461171.8407,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.6974+40.0274 20260511.3407 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 11.3407 2461171.8407 12.34 22:01:55.46 +41:18:33.7
91.86882 -11.11835 galactic Lac Second-epoch detections are separated by 1.5" 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 | 22:01:55.46 +41:18:33.7 (user input) | T | P | (position from user input) J-Ks=0.509+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:01:55.46 +41:18:33.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:01:55.46 +41:18:33.7: 14.84 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.84 +/- 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,2461171.8407,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.33 21:34:53.21 +38:42:28.1
86.14798 -9.74253 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 | 21:34:53.21 +38:42:28.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:53.21 +38:42:28.1: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:53.21 +38:42:28.1: 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,2461171.8407,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.21 21:39:45.87 +39:07:09.7
87.13973 -10.08192 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 J324.9362+39.1311 | 21:39:47.40 +39:07:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.049 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:45.87 +39:07:09.7: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:45.87 +39:07:09.7: 14.42 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.9362+39.1311,2461171.8407,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.9362+39.1311 20260511.3407 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 11.3407 2461171.8407 12.39 21:51:49.78 +37:26:01.7
87.82842 -12.90875 galactic Cyg Second-epoch detections are separated by 0.3" and 7.2 pix
The object was found in VSX20" STSP J215151.42+372556.3
Type: EA
# Max. Min./Amp. JD0 Period
17.490 r 17.910 r 2458714.80500 5.787900000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:49.78 +37:26:01.7: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:49.78 +37:26:01.7: 14.95 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STSP J215151.42+372556.3,2461171.8407,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STSP J215151.42+372556.3 20260511.3407 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 11.3407 2461171.8407 12.43 21:35:04.43 +35:48:30.7
84.15339 -11.88012 galactic Cyg Second-epoch detections are separated by 1.9" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1951001749052505088
Type: ROT
# Max. Min./Amp. JD0 Period
14.450 G 14.490 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:04.43 +35:48:30.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:04.43 +35:48:30.7: 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
Gaia DR3 1951001749052505088,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1951001749052505088 20260511.3407 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 11.3407 2461171.8407 12.32 21:54:13.73 +42:03:13.6
91.19377 -9.64266 galactic Cyg 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 | target | 21:54:13.73 +42:03:13.6 (user input) | T | P | (position from user input) J-Ks=0.806+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:13.73 +42:03:13.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:13.73 +42:03:13.6: 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,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.51 21:33:15.84 +41:05:44.8
87.56870 -7.78604 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 | target | 21:33:15.84 +41:05:44.8 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:15.84 +41:05:44.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:15.84 +41:05:44.8: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.32 21:36:45.81 +37:27:45.6
85.55974 -10.90521 galactic Cyg Second-epoch detections are separated by 2.5" 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 | 21:36:45.81 +37:27:45.6 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.047 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:45.81 +37:27:45.6: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:45.81 +37:27:45.6: 14.95 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.25 21:53:17.78 +39:27:52.6
89.38547 -11.53362 galactic Cyg Second-epoch detections are separated by 4.0" 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 | 21:53:17.78 +39:27:52.6 (user input) | T | P | (position from user input) J-Ks=0.875+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:17.78 +39:27:52.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:17.78 +39:27:52.6: 14.89 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.89 +/- 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,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.39 21:43:25.56 +36:45:53.3
86.08235 -12.31556 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 21:43:25.56 +36:45:53.3 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.044 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:25.56 +36:45:53.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:25.56 +36:45:53.3: 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
target,2461171.8407,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.51 21:33:43.13 +37:03:45.9
84.83136 -10.78219 galactic Cyg Second-epoch detections are separated by 2.5" 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 | ATO J323.4299+37.0630 | 21:33:43.13 +37:03:45.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.449+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:43.13 +37:03:45.9: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:43.13 +37:03:45.9: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.4299+37.0630,2461171.8407,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.4299+37.0630 20260511.3407 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 11.3407 2461171.8407 12.54 21:35:22.67 +38:34:23.4
86.12584 -9.90637 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 | ATO J323.8476+38.5796 | 21:35:22.67 +38:34:23.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:22.67 +38:34:23.4: 13.27 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:22.67 +38:34:23.4: 14.91 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.8476+38.5796,2461171.8407,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.8476+38.5796 20260511.3407 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.45 21:30:52.00 +36:48:41.6
84.23567 -10.56945 galactic Cyg Second-epoch detections are separated by 2.1" and 7.2 pix
The object was found in VSX19" ZTF J213051.98+364822.8
Type: EW
# Max. Min./Amp. JD0 Period
19.399 r Y 0.799 r 2458582.96430 0.260603000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:52.00 +36:48:41.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:52.00 +36:48:41.6: 15.10 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213051.98+364822.8,2461171.8407,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213051.98+364822.8 20260511.3407 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 11.3407 2461171.8407 12.35 21:26:29.45 +38:23:36.6
84.72775 -8.83212 galactic Cyg Second-epoch detections are separated by 2.5" and 7.1 pix
The object was found in VSX25" Gaia DR3 1964450459889903488
Type: ROT
# Max. Min./Amp. JD0 Period
15.760 G 15.820 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:29.45 +38:23:36.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:29.45 +38:23:36.6: 14.66 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1964450459889903488,2461171.8407,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1964450459889903488 20260511.3407 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 11.3407 2461171.8407 12.36 21:31:04.46 +38:40:10.2
85.57339 -9.25900 galactic Cyg 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 | 21:31:04.46 +38:40:10.2 (user input) | T | P | (position from user input) J-Ks=0.743+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:04.46 +38:40:10.2: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:04.46 +38:40:10.2: 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,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.47 21:26:33.88 +37:40:38.8
84.22865 -9.35180 galactic Cyg 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 | ATO J321.6417+37.6779 | 21:26:33.88 +37:40:38.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.370+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:26:33.88 +37:40:38.8: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:26:33.88 +37:40:38.8: 14.87 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.6417+37.6779,2461171.8407,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.6417+37.6779 20260511.3407 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 11.3407 2461171.8407 12.28 21:59:56.14 +38:33:11.3
89.82420 -13.05362 galactic Lac Second-epoch detections are separated by 1.4" and 7.3 pix
The object was found in VSX 3" Gaia DR3 1956022943776768128
Type: E
# Max. Min./Amp. JD0 Period
14.650 G 14.880 G 4.413330000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:56.14 +38:33:11.3: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:56.14 +38:33:11.3: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956022943776768128,2461171.8407,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956022943776768128 20260511.3407 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 11.3407 2461171.8407 12.30 21:33:02.70 +37:08:25.1
84.78661 -10.63341 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 21:33:02.70 +37:08:25.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:02.70 +37:08:25.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:02.70 +37:08:25.1: 14.51 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.51 +/- 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,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:42:26.91 +41:38:32.4
89.22854 -8.53988 galactic Cyg Second-epoch detections are separated by 2.8" 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 | 21:42:26.91 +41:38:32.4 (user input) | T | P | (position from user input) J-Ks=0.680+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:26.91 +41:38:32.4: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:26.91 +41:38:32.4: 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
target,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.38 21:47:16.33 +40:11:10.3
88.95770 -10.23672 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 | ATO J326.8262+40.1893 | 21:47:16.33 +40:11:10.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:16.33 +40:11:10.3: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:16.33 +40:11:10.3: 15.00 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.00 +/- 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 J326.8262+40.1893,2461171.8407,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.8262+40.1893 20260511.3407 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 11.3407 2461171.8407 12.36 21:31:06.05 +36:31:15.7
84.06456 -10.81099 galactic Cyg 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 | ATO J322.7654+36.5145 | 21:31:06.05 +36:31:15.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.480+/-0.048 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:31:06.05 +36:31:15.7: 12.72 +/- 0.18 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:31:06.05 +36:31:15.7: 14.96 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.7654+36.5145,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.7654+36.5145 20260511.3407 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 11.3407 2461171.8407 12.45 21:45:33.11 +39:44:22.6
88.40749 -10.35933 galactic Cyg Second-epoch detections are separated by 0.9" 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 | target | 21:45:33.11 +39:44:22.6 (user input) | T | P | (position from user input) J-Ks=0.672+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:33.11 +39:44:22.6: 13.43 +/- 0.29 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:33.11 +39:44:22.6: 15.51 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.43 +/- 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,2461171.8407,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.38 21:30:48.43 +33:38:08.4
81.96333 -12.83575 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 | target | 21:30:48.43 +33:38:08.4 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.046 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:48.43 +33:38:08.4: 13.41 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:48.43 +33:38:08.4: 15.19 +/- 0.32 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461171.8407,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.42 21:27:45.97 +37:48:40.8
84.49540 -9.42308 galactic Cyg Second-epoch detections are separated by 2.0" 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 | target | 21:27:45.97 +37:48:40.8 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:27:45.97 +37:48:40.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:27:45.97 +37:48:40.8: 14.88 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.52 21:43:40.18 +40:38:45.6
88.73763 -9.44012 galactic Cyg Second-epoch detections are separated by 1.5" 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 | 21:43:40.18 +40:38:45.6 (user input) | T | P | (position from user input) J-Ks=0.797+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:40.18 +40:38:45.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:40.18 +40:38:45.6: 15.17 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.57 21:32:42.44 +36:55:39.2
84.58757 -10.74087 galactic Cyg 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 | 21:32:42.44 +36:55:39.2 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:42.44 +36:55:39.2: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:42.44 +36:55:39.2: 15.05 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.47 21:40:59.68 +40:51:38.8
88.49724 -8.94368 galactic Cyg Second-epoch detections are separated by 1.8" and 6.8 pix
The object was found in VSX 1" ASASSN-V J214059.56+405138.3
Type: ROT
# Max. Min./Amp. JD0 Period
15.340 g Y 0.320 g 2459496.63800 9.607000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:59.68 +40:51:38.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:59.68 +40:51:38.8: 15.27 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214059.56+405138.3,2461171.8407,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214059.56+405138.3 20260511.3407 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 11.3407 2461171.8407 12.37 21:41:36.39 +36:01:13.3
85.29351 -12.62379 galactic Cyg Second-epoch detections are separated by 2.6" 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 | 21:41:36.39 +36:01:13.3 (user input) | T | P | (position from user input) J-Ks=0.606+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:41:36.39 +36:01:13.3: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:41:36.39 +36:01:13.3: 14.92 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.92 +/- 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,2461171.8407,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.24 21:43:18.85 +42:12:55.3
89.73283 -8.21526 galactic Cyg Second-epoch detections are separated by 2.3" 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 | 21:43:18.85 +42:12:55.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:18.85 +42:12:55.3: 13.00 +/- 0.23 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:18.85 +42:12:55.3: 14.66 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461171.8407,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.36 21:59:55.38 +41:14:21.2
91.52257 -10.94279 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 J329.9890+41.2310 | 21:59:55.38 +41:14:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.814+/-0.032 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:55.38 +41:14:21.2: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:55.38 +41:14:21.2: 15.37 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.9890+41.2310,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.9890+41.2310 20260511.3407 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 11.3407 2461171.8407 12.20 21:32:28.57 +41:35:15.2
87.79928 -7.32619 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 J323.1207+41.5990 | 21:32:28.57 +41:35:15.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:28.57 +41:35:15.2: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:28.57 +41:35:15.2: 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 J323.1207+41.5990,2461171.8407,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.1207+41.5990 20260511.3407 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 11.3407 2461171.8407 12.32 21:40:19.51 +35:38:54.4
84.83996 -12.72360 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 | 21:40:19.51 +35:38:54.4 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.667+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:19.51 +35:38:54.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:19.51 +35:38:54.4: 14.70 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.70 +/- 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,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.07 22:02:22.53 +41:34:46.7
92.10516 -10.95590 galactic Lac Second-epoch detections are separated by 0.6" 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 | 22:02:22.53 +41:34:46.7 (user input) | T | P | (position from user input) J-Ks=0.752+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:22.53 +41:34:46.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:22.53 +41:34:46.7: 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,2461171.8407,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.34 21:47:40.82 +39:31:35.5
88.58138 -10.78844 galactic Cyg Second-epoch detections are separated by 0.6" 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 | 21:47:40.82 +39:31:35.5 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:40.82 +39:31:35.5: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:40.82 +39:31:35.5: 14.84 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.84 +/- 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,2461171.8407,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.57 21:40:21.14 +39:47:14.2
87.67929 -9.66189 galactic Cyg Second-epoch detections are separated by 2.5" 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 | target | 21:40:21.14 +39:47:14.2 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.046 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:21.14 +39:47:14.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:21.14 +39:47:14.2: 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
target,2461171.8407,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.27 21:46:33.41 +36:26:40.7
86.34702 -12.97176 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 | target | 21:46:33.41 +36:26:40.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.500+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:33.41 +36:26:40.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:33.41 +36:26:40.7: 14.86 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.86 +/- 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,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.51 21:39:51.01 +41:51:15.6
89.00450 -8.05960 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 | 21:39:51.01 +41:51:15.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.814+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:51.01 +41:51:15.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:51.01 +41:51:15.6: 15.04 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.43 21:42:58.43 +36:37:09.6
85.91390 -12.36350 galactic Cyg Second-epoch detections are separated by 2.1" and 7.2 pix
The object was found in VSX 2" Gaia DR3 1952413071005742848
Type: ROT
# Max. Min./Amp. JD0 Period
14.970 G 15.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:58.43 +36:37:09.6: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:58.43 +36:37:09.6: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1952413071005742848,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952413071005742848 20260511.3407 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 11.3407 2461171.8407 12.25 22:02:54.66 +40:29:56.2
91.51440 -11.87393 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 | target | 22:02:54.66 +40:29:56.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:54.66 +40:29:56.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:54.66 +40:29:56.2: 15.07 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.07 +/- 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,2461171.8407,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.19 21:40:44.23 +35:27:42.4
84.77404 -12.91786 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 21:40:44.23 +35:27:42.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.651+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:44.23 +35:27:42.4: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:44.23 +35:27:42.4: 15.12 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.24 21:29:46.84 +38:09:45.8
85.03218 -9.44837 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 J322.4316+38.1632 | 21:29:46.84 +38:09:45.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.570+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:46.84 +38:09:45.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:46.84 +38:09:45.8: 14.58 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.4316+38.1632,2461171.8407,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.4316+38.1632 20260511.3407 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 11.3407 2461171.8407 12.47 21:28:45.90 +38:15:12.3
84.95107 -9.24434 galactic Cyg 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 | ATO J322.2043+38.2607 | 21:28:45.90 +38:15:12.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.391+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:45.90 +38:15:12.3: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:45.90 +38:15:12.3: 15.31 +/- 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 J322.2043+38.2607,2461171.8407,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.2043+38.2607 20260511.3407 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 11.3407 2461171.8407 12.54 21:33:20.63 +39:12:48.5
86.27707 -9.16855 galactic Cyg Second-epoch detections are separated by 2.3" 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 | 21:33:20.63 +39:12:48.5 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:33:20.63 +39:12:48.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:33:20.63 +39:12:48.5: 14.62 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.36 21:32:07.67 +37:19:42.8
84.78450 -10.37119 galactic Cyg Second-epoch detections are separated by 1.5" 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 | 21:32:07.67 +37:19:42.8 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.051 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:07.67 +37:19:42.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:07.67 +37:19:42.8: 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,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.46 21:42:46.32 +41:48:21.2
89.38358 -8.45692 galactic Cyg Second-epoch detections are separated by 2.7" 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 | target | 21:42:46.32 +41:48:21.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:46.32 +41:48:21.2: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:46.32 +41:48:21.2: 15.16 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.16 +/- 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,2461171.8407,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.39 21:49:46.22 +40:24:27.8
89.47241 -10.37648 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 | 21:49:46.22 +40:24:27.8 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:46.22 +40:24:27.8: 13.53 +/- 0.31 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:46.22 +40:24:27.8: 14.98 +/- 0.23 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,2461171.8407,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.34 21:32:41.24 +35:18:25.0
83.44067 -11.90782 galactic Cyg 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 | ATO J323.1712+35.3046 | 21:32:41.24 +35:18:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:32:41.24 +35:18:25.0: 12.94 +/- 0.19 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:32:41.24 +35:18:25.0: 15.12 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 J323.1712+35.3046,2461171.8407,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.1712+35.3046 20260511.3407 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 11.3407 2461171.8407 12.28 21:45:06.37 +36:34:15.4
86.20832 -12.68430 galactic Cyg Second-epoch detections are separated by 5.0" 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 | target | 21:45:06.37 +36:34:15.4 (user input) | T | P | (position from user input) J-Ks=0.511+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:06.37 +36:34:15.4: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:06.37 +36:34:15.4: 14.83 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:43:09.00 +34:51:35.6
84.73271 -13.69493 galactic Cyg Second-epoch detections are separated by 0.9" and 7.2 pix
The object was found in VSX 3" Gaia DR3 1947754749475643904
Type: ROT
# Max. Min./Amp. JD0 Period
14.770 G 14.820 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:09.00 +34:51:35.6: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:09.00 +34:51:35.6: 14.69 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1947754749475643904,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1947754749475643904 20260511.3407 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 11.3407 2461171.8407 12.38 21:45:12.21 +40:36:36.9
88.93619 -9.65837 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 | 21:45:12.21 +40:36:36.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:12.21 +40:36:36.9: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:12.21 +40:36:36.9: 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,2461171.8407,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.31 21:49:25.05 +42:02:02.8
90.48300 -9.08905 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 | 21:49:25.05 +42:02:02.8 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:25.05 +42:02:02.8: 12.86 +/- 0.20 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:25.05 +42:02:02.8: 15.04 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461171.8407,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.18 21:45:58.77 +39:55:46.8
88.59711 -10.26957 galactic Cyg Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 2" Gaia DR3 1954120926101711872
Type: ROT
# Max. Min./Amp. JD0 Period
14.530 G 14.550 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:58.77 +39:55:46.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:58.77 +39:55:46.8: 14.72 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1954120926101711872,2461171.8407,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1954120926101711872 20260511.3407 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 11.3407 2461171.8407 12.35 21:50:22.55 +40:29:51.6
89.62088 -10.38177 galactic Cyg 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 | 21:50:22.55 +40:29:51.6 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.037 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:22.55 +40:29:51.6: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:22.55 +40:29:51.6: 15.15 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.15 +/- 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,2461171.8407,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:34:38.98 +38:53:37.6
86.24260 -9.57514 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 21:34:38.98 +38:53:37.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.362+/-0.034 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:38.98 +38:53:37.6: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:38.98 +38:53:37.6: 14.41 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.48 21:39:22.59 +41:40:38.5
88.81875 -8.13240 galactic Cyg Second-epoch detections are separated by 1.9" 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 | 21:39:22.59 +41:40:38.5 (user input) | T | P | (position from user input) J-Ks=0.845+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:22.59 +41:40:38.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:22.59 +41:40:38.5: 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,2461171.8407,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.38 21:40:31.69 +41:13:38.5
88.67777 -8.61158 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 | target | 21:40:31.69 +41:13:38.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.822+/-0.030 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:31.69 +41:13:38.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:31.69 +41:13:38.5: 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
target,2461171.8407,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.26 21:45:08.22 +34:07:00.6
84.53369 -14.52107 galactic Cyg Second-epoch detections are separated by 1.6" 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 | 21:45:08.22 +34:07:00.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:08.22 +34:07:00.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:08.22 +34:07:00.6: 15.12 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.12 +/- 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,2461171.8407,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:46:37.51 +40:59:09.7
89.39180 -9.54973 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 | target | 21:46:37.51 +40:59:09.7 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:37.51 +40:59:09.7: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:37.51 +40:59:09.7: 14.92 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.92 +/- 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,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.29 21:51:16.57 +41:52:17.0
90.64622 -9.43539 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 | target | 21:51:16.57 +41:52:17.0 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.051 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:16.57 +41:52:17.0: 13.22 +/- 0.24 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:16.57 +41:52:17.0: 15.31 +/- 0.32 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461171.8407,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.44 21:28:44.78 +40:00:03.1
86.17909 -7.98758 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 21:28:44.78 +40:00:03.1 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:44.78 +40:00:03.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:44.78 +40:00:03.1: 15.10 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.43 21:28:54.40 +40:16:40.9
86.39577 -7.80954 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 21:28:54.40 +40:16:40.9 (user input) | T | P | (position from user input) J-Ks=0.495+/-0.036 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:28:54.40 +40:16:40.9: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:28:54.40 +40:16:40.9: 14.78 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.78 +/- 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,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.46 21:37:02.71 +36:17:37.7
84.78959 -11.79923 galactic Cyg 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 | 21:37:02.71 +36:17:37.7 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:02.71 +36:17:37.7: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:02.71 +36:17:37.7: 14.95 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.40 21:34:21.84 +35:35:52.5
83.89840 -11.93371 galactic Cyg Second-epoch detections are separated by 2.6" 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 J323.5910+35.5987 | 21:34:21.84 +35:35:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:21.84 +35:35:52.5: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:21.84 +35:35:52.5: 14.80 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.5910+35.5987,2461171.8407,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.5910+35.5987 20260511.3407 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 11.3407 2461171.8407 12.30 21:59:29.16 +39:40:32.7
90.46863 -12.11965 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 | 21:59:29.16 +39:40:32.7 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.045 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:59:29.16 +39:40:32.7: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:59:29.16 +39:40:32.7: 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
target,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.41 21:34:26.47 +39:32:18.8
86.65898 -9.07659 galactic Cyg Second-epoch detections are separated by 3.0" and 6.8 pix
The object was found in VSX 3" Gaia DR3 1965881130673926400
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.870 G 14.910 G 0.092812500000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:26.47 +39:32:18.8: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:26.47 +39:32:18.8: 15.15 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1965881130673926400,2461171.8407,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965881130673926400 20260511.3407 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 11.3407 2461171.8407 12.34 21:39:30.80 +37:21:42.4
85.89941 -11.34935 galactic Cyg Second-epoch detections are separated by 2.8" 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 | 21:39:30.80 +37:21:42.4 (user input) | T | P | (position from user input) J-Ks=0.871+/-0.034 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:39:30.80 +37:21:42.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:39:30.80 +37:21:42.4: 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,2461171.8407,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.47 21:50:42.00 +37:37:59.1
87.78503 -12.61197 galactic Cyg Second-epoch detections are separated by 3.1" 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 | 21:50:42.00 +37:37:59.1 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.039 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:42.00 +37:37:59.1: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:42.00 +37:37:59.1: 15.33 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.33 +/- 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,2461171.8407,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.37 21:46:04.17 +39:02:58.2
88.02373 -10.94587 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 | target | 21:46:04.17 +39:02:58.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.813+/-0.035 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:04.17 +39:02:58.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:04.17 +39:02:58.2: 15.47 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.47 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.49 21:36:40.49 +40:02:26.4
87.32325 -9.00005 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 | ATO J324.1541+40.0418 | 21:36:40.49 +40:02:26.4 (user input) | SINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:36:40.49 +40:02:26.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:36:40.49 +40:02:26.4: 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
ATO J324.1541+40.0418,2461171.8407,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.1541+40.0418 20260511.3407 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 11.3407 2461171.8407 12.50 21:29:56.43 +36:57:31.6
84.20461 -10.33485 galactic Cyg Second-epoch detections are separated by 1.8" and 7.5 pix
The object was found in VSX 2" Gaia DR3 1952101982234823680
Type: ROT
# Max. Min./Amp. JD0 Period
14.630 G 14.670 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:56.43 +36:57:31.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:56.43 +36:57:31.6: 15.12 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.12 +/- 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
Gaia DR3 1952101982234823680,2461171.8407,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952101982234823680 20260511.3407 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.30 21:37:40.29 +36:45:52.0
85.21089 -11.54018 galactic Cyg Second-epoch detections are separated by 0.7" 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 | target | 21:37:40.29 +36:45:52.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:40.29 +36:45:52.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:40.29 +36:45:52.0: 14.53 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.53 +/- 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,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.26 21:40:19.70 +35:37:23.5
84.82296 -12.74265 galactic Cyg Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX17" Gaia DR3 1950852765226527104
Type: ROT
# Max. Min./Amp. JD0 Period
17.130 G 17.160 G 0.454966000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:19.70 +35:37:23.5: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:19.70 +35:37:23.5: 15.25 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.25 +/- 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
Gaia DR3 1950852765226527104,2461171.8407,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1950852765226527104 20260511.3407 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 11.3407 2461171.8407 12.27 21:48:39.15 +37:49:35.0
87.59828 -12.20209 galactic Cyg Second-epoch detections are separated by 0.7" 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 | target | 21:48:39.15 +37:49:35.0 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:48:39.15 +37:49:35.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:48:39.15 +37:49:35.0: 15.20 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.20 +/- 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,2461171.8407,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.54 21:54:20.83 +39:10:07.1
89.35342 -11.89129 galactic Cyg 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 | 21:54:20.83 +39:10:07.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:54:20.83 +39:10:07.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:54:20.83 +39:10:07.1: 15.28 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.28 +/- 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,2461171.8407,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.65 21:34:43.80 +39:32:52.7
86.70671 -9.10771 galactic Cyg Second-epoch detections are separated by 2.4" and 7.3 pix
The object was found in VSX 1" Gaia DR3 1965881336832478336
Type: E
# Max. Min./Amp. JD0 Period
14.870 G 15.180 G 0.726630000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:43.80 +39:32:52.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:43.80 +39:32:52.7: 15.04 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.04 +/- 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
Gaia DR3 1965881336832478336,2461171.8407,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1965881336832478336 20260511.3407 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.47 21:34:30.95 +37:25:09.5
85.19795 -10.63206 galactic Cyg Second-epoch detections are separated by 2.7" and 7.1 pix
The object was found in VSX 2" Gaia DR3 1952178741889098624
Type: ROT
# Max. Min./Amp. JD0 Period
14.640 G 14.680 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:34:30.95 +37:25:09.5: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:34:30.95 +37:25:09.5: 15.39 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.39 +/- 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
Gaia DR3 1952178741889098624,2461171.8407,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1952178741889098624 20260511.3407 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 11.3407 2461171.8407 12.51 21:45:41.64 +42:01:42.6
89.94611 -8.64554 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 J326.4062+42.0284 | 21:45:41.64 +42:01:42.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.503+/-0.046 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:41.64 +42:01:42.6: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:41.64 +42:01:42.6: 15.38 +/- 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 J326.4062+42.0284,2461171.8407,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.4062+42.0284 20260511.3407 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 11.3407 2461171.8407 12.48 21:29:12.22 +35:45:11.1
83.23934 -11.09391 galactic Cyg 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 | 21:29:12.22 +35:45:11.1 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:29:12.22 +35:45:11.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:29:12.22 +35:45:11.1: 14.74 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.60 21:47:00.98 +41:24:09.3
89.72317 -9.28128 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 21:47:00.98 +41:24:09.3 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.039 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:00.98 +41:24:09.3: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:00.98 +41:24:09.3: 15.16 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.60CV 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 11.3407 2461171.8407 12.32 21:49:57.53 +36:11:59.4
86.71384 -13.60583 galactic Peg 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 | ATO J327.4838+36.2070 | 21:49:57.53 +36:11:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.595+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:57.53 +36:11:59.4: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:57.53 +36:11:59.4: 15.32 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.32 +/- 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 J327.4838+36.2070,2461171.8407,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4838+36.2070 20260511.3407 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 11.3407 2461171.8407 12.49 21:44:11.75 +40:40:16.9
88.83069 -9.48675 galactic Cyg Second-epoch detections are separated by 1.9" 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 | 21:44:11.75 +40:40:16.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:11.75 +40:40:16.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:11.75 +40:40:16.9: 15.19 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.19 +/- 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,2461171.8407,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.44 21:45:54.45 +37:57:42.2
87.27050 -11.74516 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 | target | 21:45:54.45 +37:57:42.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:45:54.45 +37:57:42.2: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:45:54.45 +37:57:42.2: 15.50 +/- 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,2461171.8407,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.30 21:40:51.91 +37:15:12.2
86.02789 -11.61041 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 | 21:40:51.91 +37:15:12.2 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.038 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:51.91 +37:15:12.2: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:51.91 +37:15:12.2: 15.15 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.49 21:42:52.72 +36:02:59.3
85.50935 -12.77437 galactic Cyg 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 | 21:42:52.72 +36:02:59.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:42:52.72 +36:02:59.3: 13.40 +/- 0.32 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:42:52.72 +36:02:59.3: 15.45 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.40 +/- 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,2461171.8407,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.43 21:40:55.96 +35:39:12.4
84.93679 -12.80321 galactic Cyg 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 | 21:40:55.96 +35:39:12.4 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.705+/-0.034 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:55.96 +35:39:12.4: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:55.96 +35:39:12.4: 15.25 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.25 +/- 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,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.43 21:44:21.52 +38:41:36.0
87.52958 -10.99483 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 | target | 21:44:21.52 +38:41:36.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:21.52 +38:41:36.0: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:21.52 +38:41:36.0: 15.29 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.29 +/- 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,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.46 21:37:04.90 +35:55:01.1
84.53231 -12.07976 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 21:37:04.90 +35:55:01.1 (user input) | T | P | (position from user input) J-Ks=0.634+/-0.040 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:37:04.90 +35:55:01.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:37:04.90 +35:55:01.1: 14.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.81 +/- 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,2461171.8407,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.50 21:52:31.17 +41:00:05.7
90.26571 -10.25411 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 | target | 21:52:31.17 +41:00:05.7 (user input) | T | P | (position from user input) J-Ks=0.938+/-0.031 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:52:31.17 +41:00:05.7: 13.62 +/- 0.34 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:52:31.17 +41:00:05.7: 15.56 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.62 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.36 21:30:32.98 +34:04:08.9
82.23555 -12.48903 galactic Cyg Second-epoch detections are separated by 1.6" 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 | 21:30:32.98 +34:04:08.9 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.042 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:30:32.98 +34:04:08.9: 13.39 +/- 0.36 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:30:32.98 +34:04:08.9: 14.73 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.41 +/- 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,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.48 21:35:25.02 +37:18:31.0
85.25359 -10.83536 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 | target | 21:35:25.02 +37:18:31.0 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.037 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:35:25.02 +37:18:31.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:35:25.02 +37:18:31.0: 15.16 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.51 21:49:21.18 +40:59:12.5
89.79009 -9.88273 galactic Cyg 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 | 21:49:21.18 +40:59:12.5 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.041 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:21.18 +40:59:12.5: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:21.18 +40:59:12.5: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.51 21:44:25.53 +41:41:20.2
89.54069 -8.74789 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 J326.1049+41.6874 | 21:44:25.53 +41:41:20.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.883+/-0.033 (M)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:25.53 +41:41:20.2: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:25.53 +41:41:20.2: 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
ATO J326.1049+41.6874,2461171.8407,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1049+41.6874 20260511.3407 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 11.3407 2461171.8407 12.28 21:58:49.47 +40:28:43.1
90.87645 -11.41166 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 | 21:58:49.47 +40:28:43.1 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.043 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:58:49.47 +40:28:43.1: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:58:49.47 +40:28:43.1: 14.99 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.99 +/- 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,2461171.8407,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.37 21:50:07.66 +42:10:52.1
90.68086 -9.06086 galactic Cyg Second-epoch detections are separated by 1.8" 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 J327.5325+42.1739 | 21:50:07.66 +42:10:52.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.441+/-0.035 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:50:07.66 +42:10:52.1: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:50:07.66 +42:10:52.1: 14.65 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.5325+42.1739,2461171.8407,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.5325+42.1739 20260511.3407 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 11.3407 2461171.8407 12.30 21:43:52.27 +38:47:06.8
87.51881 -10.86304 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 J325.9684+38.7838 | 21:43:52.27 +38:47:06.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.454+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:43:52.27 +38:47:06.8: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:43:52.27 +38:47:06.8: 14.72 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 J325.9684+38.7838,2461171.8407,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.9684+38.7838 20260511.3407 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 11.3407 2461171.8407 12.50 21:51:02.72 +40:49:27.0
89.93279 -10.21281 galactic Cyg Second-epoch detections are separated by 0.7" and 7.1 pix
The object was found in VSX20" Gaia DR3 1960221222769156736
Type: VAR
# Max. Min./Amp. JD0 Period
15.990 G 16.020 G 0.018186700000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:02.72 +40:49:27.0: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:02.72 +40:49:27.0: 15.38 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.38 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1960221222769156736,2461171.8407,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960221222769156736 20260511.3407 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 11.3407 2461171.8407 12.41 21:46:33.45 +37:56:10.3
87.35201 -11.84863 galactic Cyg Second-epoch detections are separated by 3.5" 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 | 21:46:33.45 +37:56:10.3 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.043 (K)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:46:33.45 +37:56:10.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:46:33.45 +37:56:10.3: 15.28 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.36 22:00:27.78 +40:13:16.8
90.96412 -11.80699 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 | 22:00:27.78 +40:13:16.8 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.041 (F)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:00:27.78 +40:13:16.8: 13.66 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:00:27.78 +40:13:16.8: 15.45 +/- 0.36 detection
Forced photometry reference-image weighted average: 14.53 +/- 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,2461171.8407,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.43 21:49:29.08 +36:55:04.2
87.12028 -12.99909 galactic Cyg 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 | target | 21:49:29.08 +36:55:04.2 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.049 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:49:29.08 +36:55:04.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:49:29.08 +36:55:04.2: 14.76 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461171.8407,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260511.3407 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 11.3407 2461171.8407 12.48 22:02:20.88 +39:30:33.9
90.80773 -12.59075 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 1956169415041419264 | 22:02:18.13 +39:30:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.425+/-0.040 (G)
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 22:02:20.88 +39:30:33.9: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 22:02:20.88 +39:30:33.9: 15.11 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1956169415041419264,2461171.8407,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956169415041419264 20260511.3407 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461171.84094165 11.05.2026 08:10:47.359 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 19348
Objects passed selection criteria: 19337
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 18639.5
Average stars matched: 16555.5 (88.8194 %)
Memory usage VmPeak: 125672 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 11 03:41:05 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
First image: 2461032.59795358 23.12.2025 02:20:53.189 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Last image: 2461171.84094165 11.05.2026 08:10:47.359 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 562
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 176 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): 136269
Objects passed selection criteria: 136047
Measurements per detected object (mean, median, min, max): 3.3 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 3.0 2 4
Average stars detected per image: 131538
Average stars matched: 117783 (89.5435 %)
Memory usage VmPeak: 1959788 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 11 03:46:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461171.84045278
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits was not set. Trying to guess...
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits was not set. Trying to guess...
The guess is 605 arcmin.
The guess is 605 arcmin.
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits .... Determining astrometry method...
It's a known telescope with plate solutions that are supposed to be good.
Choosing aperture...
Using the local copy of Astrometry.net software...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
It's a known telescope with plate solutions that are supposed to be good.
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits was not set. Trying to guess...
The guess is 572 arcmin.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits was not set. Trying to guess...
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
The guess is 570 arcmin.
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits was not found.
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/lib/make_outxyls_for_astrometric_calibration found 20482 high-SNR stars for plate solving
Generating wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat from image00001.cat
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/lib/make_outxyls_for_astrometric_calibration found 20749 high-SNR stars for plate solving
Generating wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat from image00002.cat
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits created.
verification OK: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits created.
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Image size: 932.3'x637.3' 15.5(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.99"/pix along the Y axis
Image center: 21:48:57.820 +38:02:09.57 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:06.050 +38:00:21.02 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Using the local copy of Astrometry.net code
### Converted positions of 28429 stars ###
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
Reading input file 1 of 1: "out912498.xyls"...
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out912501.xyls"...
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
### Converted positions of 21746 stars ###
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/correct_sextractor_wcs_catalog_usingxy2sky912880.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/correct_sextractor_wcs_catalog_usingxy2sky912874.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out912498.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Reading file "./out912501.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 38.6644 (6.19094e+16), 7 match, 0 conflict, 32 distractors, 23 index.
RA,Dec = (327.271,38.0035), pixel scale 5.95807 arcsec/pix.
Hit/miss: Hit/miss: -+----+++-------------------+-+-------+(best)-------------+-----------------------------------------------
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out912498.solved to indicate this.
Field 1 did not solve (index index-4115.fits, field objects 1-10).
log-odds ratio 30.0038 (1.07275e+13), 6 match, 0 conflict, 19 distractors, 96 index.
RA,Dec = (327.234,38.0148), pixel scale 5.9076 arcsec/pix.
Hit/miss: Hit/miss: +----+------+---+---+---+(best)-------+-------+---+-------+---+-----------+-------++----------+-----------
Field: out912498.xyls
Field center: (RA,Dec) = (327.279169, 38.003364) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:07.000, +38:00:12.109).
Field size: 15.7384 x 10.5275 degrees
Field rotation angle: up is -0.976244 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits' -> 'fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits'
Field 1: solved with index index-4114.fits.
Field 1 solved: writing to file ./out912501.solved to indicate this.
Field: out912501.xyls
Field center: (RA,Dec) = (327.293687, 38.005620) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:10.485, +38:00:20.232).
Field size: 15.7351 x 10.5303 degrees
Field rotation angle: up is -0.963037 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits' -> 'fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 03:41 fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
-rw-r--r-- 1 apache apache 12K May 11 03:41 out912498.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits)... done!
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 03:41 fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
-rw-r--r-- 1 apache apache 12K May 11 03:41 out912501.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits)... done!
done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits (fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits (fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out912498.xyls"...
Reading input file 1 of 1: "out912501.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out912498.axy"...
Only searching for solutions within 15.6667 degrees of RA,Dec (327.28,38.0042)
log-odds ratio 38.6644 (6.19094e+16), 7 match, 0 conflict, 32 distractors, 23 index.
RA,Dec = (327.271,38.0035), pixel scale 5.95807 arcsec/pix.
Hit/miss: Hit/miss: -+----+++-------------------+-+-------+(best)-------------+-----------------------------------------------
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out912501.axy"...
Only searching for solutions within 15.6667 degrees of RA,Dec (327.295,38.0065)
log-odds ratio 39.3613 (1.24272e+17), 8 match, 0 conflict, 39 distractors, 23 index.
RA,Dec = (327.285,38.0083), pixel scale 5.95806 arcsec/pix.
Hit/miss: Hit/miss: -+----+++-----------------+---+-------+-------+(best)-----------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out912498.solved to indicate this.
Field: out912498.xyls
Field center: (RA,Dec) = (327.282694, 38.001505) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:07.847, +38:00:05.416).
Field size: 15.7165 x 10.5367 degrees
Field rotation angle: up is -0.983309 degrees E of N
Field parity: neg
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out912501.solved to indicate this.
Field: out912501.xyls
Field center: (RA,Dec) = (327.296776, 38.006174) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:11.226, +38:00:22.225).
Field size: 15.7161 x 10.5371 degrees
Field rotation angle: up is -0.979956 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 03:41 fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
-rw-r--r-- 1 apache apache 12K May 11 03:41 out912498.wcs
Inserting WCS header (2nd iteration local)...
Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits)... done!
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 03:41 fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
-rw-r--r-- 1 apache apache 12K May 11 03:41 out912501.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits for reading... done!
Creating new image file (wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits)... done!
done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 96900 sources.
simplexy: found 100000 sources.
Solving...
Solving...
Reading file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.axy"...
Verifying WCS using indices with quads of size [63.5026, 951.943] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 236.774 (6.75578e+102), 32 match, 0 conflict, 172 distractors, 49 index.
RA,Dec = (327.282,38.0007), pixel scale 5.96455 arcsec/pix.
Hit/miss: Hit/miss: -------+------------++------++------+------+-------+---+---+----+--+-+----+-+-----------+--+--------
--> log-odds 236.774
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 543.889 (1.61498e+236), 61 match, 0 conflict, 188 distractors, 99 index.
RA,Dec = (327.282,38.0007), pixel scale 5.96455 arcsec/pix.
Hit/miss: Hit/miss: --++-+++--+-+-++-+--++++--+-+++--+-++-+----+-------+---+---+----+--+-+++--+-+-----+---+-+--+-----+--
--> log-odds 543.889
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 984.783 (inf), 111 match, 0 conflict, 227 distractors, 196 index.
RA,Dec = (327.282,38.0007), pixel scale 5.96455 arcsec/pix.
Hit/miss: Hit/miss: -+++++++--++++++-+--++++--+-++++++-++-+-+-++-+---+++-+++--++--+-+-++-++++-+++-+++-+++-+++-++++++-++-
--> log-odds 984.783
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 1709.85 (inf), 197 match, 0 conflict, 204 distractors, 377 index.
RA,Dec = (327.282,38.0007), pixel scale 5.96455 arcsec/pix.
Hit/miss: Hit/miss: ++++++++--++++++-+--+++++-++++++++-++++-+-++++++-+++++++-++++++-+-++-++++-+++++++-+++-+++-++++++-++-
Reading file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.axy"...
Verifying WCS using indices with quads of size [63.5047, 951.974] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 48.5586 (1.22668e+21), 7 match, 0 conflict, 39 distractors, 23 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: ----+----++-------+---------+------+---------+(best)------------------------------------------------------
--> log-odds 1709.85
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3055.83 (inf), 384 match, 0 conflict, 503 distractors, 735 index.
RA,Dec = (327.282,38.0007), pixel scale 5.96455 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++-++++++-+++++++++++++++-++++++-+++++++-++++++++-++++++++++++++++++++++++++++++++++
--> log-odds 48.5586
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 156.346 (7.9505e+67), 26 match, 0 conflict, 194 distractors, 49 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: ----+--+-++-------+-+------++------+---------+-+-----+----+---------------------+-----+-------------
--> log-odds 156.346
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 367.937 (6.21022e+159), 47 match, 0 conflict, 195 distractors, 99 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: ---+++++-++-+-++--+-+--+--+++-----++---------+-+-----+-+--+---+---+---------+---+-----+--------+-+--
--> log-odds 3055.83
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 5753.76 (inf), 784 match, 0 conflict, 923 distractors, 1454 index.
RA,Dec = (327.282,38.0007), pixel scale 5.96455 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 367.937
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 770.052 (inf), 89 match, 0 conflict, 159 distractors, 196 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: --++++++-++++-+++-+-+--++-+++-++-+++-+----+-++-+--+-++-+-++-+-+---+--+-+--+-+-+-+-++-++--------+-++-
--> log-odds 770.052
--> log-odds 5753.76
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 1439.39 (inf), 171 match, 0 conflict, 222 distractors, 377 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: --++++++-++++-+++-+-+-+++++++-++++++++++--++++++-+++++-+-++-+++++++-++-++-+-+-+++-++-+++-++----+-++-
--> log-odds 1439.39
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 2700.66 (inf), 345 match, 0 conflict, 484 distractors, 735 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++-++++++++++++++++++++-+++++++++++++++-++++++++++++++++-+++++++++++++++++++-++++++
--> log-odds 2700.66
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 5105.05 (inf), 701 match, 0 conflict, 746 distractors, 1454 index.
RA,Dec = (327.296,38.0053), pixel scale 5.96475 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++-++++++
--> log-odds 5105.05
Got 7 solutions.
Got 6 solutions.
Field: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Field: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Field center: (RA,Dec) = (327.295815, 38.005614) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:10.996, +38:00:20.209).
Field size: 15.7203 x 10.5331 degrees
Field rotation angle: up is -0.964827 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.new"...
Field center: (RA,Dec) = (327.281744, 38.000884) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:49:07.619, +38:00:03.184).
Field size: 15.7205 x 10.5331 degrees
Field rotation angle: up is -0.968759 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.new"...
renamed 'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.new' -> 'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits'
renamed 'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.new' -> 'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits'
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits was not found.
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Generating wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat from image00004.cat
Generating wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat from image00003.cat
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits created.
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits created.
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Image size: 938.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:07.867 +38:00:06.21 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 938.0'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:11.244 +38:00:23.24 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 21484 stars ###
'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/correct_sextractor_wcs_catalog_usingxy2sky931977.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
### Converted positions of 21634 stars ###
'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/correct_sextractor_wcs_catalog_usingxy2sky931992.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (1st reference image)
verification OK: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Image size: 932.3'x637.3' 15.5(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.99"/pix along the Y axis
Image center: 21:48:57.820 +38:02:09.57 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits (1st new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Image size: 938.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:07.867 +38:00:06.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:07.867 +38:00:06.21
Angular distance between the image centers 0.0476 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits (2nd new image)
verification OK: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Image size: 938.0'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:49:11.244 +38:00:23.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:48:57.820 +38:02:09.57
Second-epoch image center 21:49:11.244 +38:00:23.24
Angular distance between the image centers 0.0530 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:49:07.867 +38:00:06.21
Second-epoch second image center 21:49:11.244 +38:00:23.24
Angular distance between the image centers 0.01205 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits &> /tmp/tmp.Vmpfln1ANb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits &> /tmp/tmp.BkM91B3O1U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits &> /tmp/tmp.tnfcCBUJcs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits &> /tmp/tmp.NMn5n0965R
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits and wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.968900
a=0.000000 b=1.000000 c=22.968900
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28429 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.8517 to 337.9501 deg, Dec +32.2173 to +43.3775 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.8517 to 337.9501 deg, Dec 32.2173 to 43.3775 deg
Loaded 21151 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 23 out of 30 total matches.
Matched with Tycho-2 30 out of 28429 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits (aperture=6.2)
Read 21746 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 316.5217 to 337.7622 deg, Dec +32.2988 to +43.2789 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 316.5217 to 337.7622 deg, Dec 32.2988 to 43.2789 deg
Loaded 21125 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 13298 out of 14228 total matches.
Matched with Tycho-2 14228 out of 21746 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits:
Forced-photometry filter: calibrated wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -> calib.txt_param_ref_wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits (aperture=7.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
2.4 pix fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
2.3 pix fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
2.2 pix wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
2.9 pix wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Limiting magnitude estimates:
15.2 mag. Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
14.7 mag. Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
14.8 mag. fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
14.9 mag. fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Vmpfln1ANb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2960, passed=28429
Got 28429 stars (including 25433 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 28429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.3'
Seting catalog search parameters based on the expected field of view 932.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012949 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010359 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 424 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 377 matched stars entering correct_measured_positions(), 326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 373 matched stars entering correct_measured_positions(), 11634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.4)
Done reading UCAC5 zone files...
Matched 495 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 453 matched stars entering correct_measured_positions(), 11686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
Accuracy estimation diagnostic: 452 matched stars entering correct_measured_positions(), 13987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
Excluding outliers - 452 stars left (next iteration limit 410)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits N_match=452 sigma_overall_arcsec=5.245 sigma_q1_arcsec=26.359 sigma_q2_arcsec=5.045 sigma_q3_arcsec=33.611 sigma_q4_arcsec=3.580 n_q1=17 n_q2=196 n_q3=13 n_q4=226 worst_quadrant_to_overall_ratio=6.408
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits -region wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BkM91B3O1U (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits' -> 'wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1940, passed=21746
Got 21746 stars (including 19798 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat
util/solve_plate_with_UCAC5 got 21746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 21214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits N_match=958 sigma_overall_arcsec=0.836 sigma_q1_arcsec=0.742 sigma_q2_arcsec=0.917 sigma_q3_arcsec=0.784 sigma_q4_arcsec=1.358 n_q1=279 n_q2=165 n_q3=306 n_q4=208 worst_quadrant_to_overall_ratio=1.625
The image catalog is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits -region wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tnfcCBUJcs (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1582, passed=21484
Got 21484 stars (including 19889 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat
util/solve_plate_with_UCAC5 got 21484 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 21133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 21132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 21132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits N_match=961 sigma_overall_arcsec=0.594 sigma_q1_arcsec=0.583 sigma_q2_arcsec=0.564 sigma_q3_arcsec=0.526 sigma_q4_arcsec=0.851 n_q1=250 n_q2=186 n_q3=295 n_q4=230 worst_quadrant_to_overall_ratio=1.434
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NMn5n0965R (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1620, passed=21634
Got 21634 stars (including 19995 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 21634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 21310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 21309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 21309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits N_match=960 sigma_overall_arcsec=0.622 sigma_q1_arcsec=0.589 sigma_q2_arcsec=0.603 sigma_q3_arcsec=0.530 sigma_q4_arcsec=0.928 n_q1=253 n_q2=185 n_q3=290 n_q4=232 worst_quadrant_to_overall_ratio=1.491
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-05_20.00sec_-4.90C_LIGHT_0381.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Cyg-07-Q2b1x1_032738_TTUQ2b1x1_230561_3AcxZQUO/wcs_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:02.33 +39:36:18.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:44:27.68 +40:44:01.1: 15.25 +/- 0.21 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:28.11 +37:51:53.4: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:56:47.58 +37:36:36.5: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:40:08.50 +38:04:10.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:00.35 +37:21:59.0: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:51:28.21 +38:11:23.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:55:39.85 +38:31:10.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:47:59.05 +38:41:49.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-07-Q2b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits at 21:53:05.38 +35:42:38.0: 15.85 +/- 0.35 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:02.33 +39:36:18.0: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.02
Forced photometry filter REJECTED candidate at 21:51:02.33 +39:36:18.0: ref_mag=12.15 +/- 0.02 new_mean_mag=12.1144 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:56:47.58 +37:36:36.5: 12.19 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:44:27.68 +40:44:01.1: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:00.35 +37:21:59.0: 12.34 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:55:39.85 +38:31:10.7: 12.24 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:28.21 +38:11:23.3: 12.21 +/- 0.02 detection
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:47:59.05 +38:41:49.5: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry reference-image weighted average: 12.34 +/- 0.02
Forced photometry filter REJECTED candidate at 21:56:47.58 +37:36:36.5: ref_mag=12.19 +/- 0.02 new_mean_mag=12.0524 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Forced photometry filter REJECTED candidate at 21:44:27.68 +40:44:01.1: ref_mag=12.28 +/- 0.02 new_mean_mag=12.2462 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Forced photometry filter REJECTED candidate at 21:53:00.35 +37:21:59.0: ref_mag=12.34 +/- 0.02 new_mean_mag=12.2065 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:55:39.85 +38:31:10.7: ref_mag=12.24 +/- 0.02 new_mean_mag=12.1438 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 12.21 +/- 0.02
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:40:08.50 +38:04:10.4: 12.03 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 21:51:28.21 +38:11:23.3: ref_mag=12.21 +/- 0.02 new_mean_mag=12.1154 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:47:59.05 +38:41:49.5: ref_mag=12.21 +/- 0.02 new_mean_mag=12.2180 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.03 +/- 0.02
Forced photometry filter REJECTED candidate at 21:40:08.50 +38:04:10.4: ref_mag=12.03 +/- 0.02 new_mean_mag=12.0958 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:51:28.11 +37:51:53.4: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter REJECTED candidate at 21:51:28.11 +37:51:53.4: ref_mag=12.25 +/- 0.02 new_mean_mag=12.1988 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cyg-07-Q2b1x1_2026-04-19_05-16-37_20.00sec_-4.90C_LIGHT_0728.fits at 21:53:05.38 +35:42:38.0: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Forced photometry filter REJECTED candidate at 21:53:05.38 +35:42:38.0: ref_mag=12.36 +/- 0.02 new_mean_mag=12.2473 delta=0.11 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 37923_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37923_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:42:59.58 +37:36:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37924_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37924_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37931_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37931_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37933_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37933_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37940_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37940_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37954_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37954_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37955_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37955_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37961_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37961_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37963_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37963_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 37987_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 37987_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 38014_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 38014_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 252943_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 252943_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 252951_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252951_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252955_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252955_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252973_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252973_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252975_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252975_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252980_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252980_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252986_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252986_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252992_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252992_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 252994_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 252994_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253002_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253002_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253029_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253029_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253033_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253033_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253034_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253034_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253042_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253042_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253078_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253078_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253082_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253082_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253087_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253087_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253088_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253088_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253095_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253095_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253096_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253096_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253111_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253111_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253123_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253123_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253124_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253124_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253131_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253131_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253135_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253135_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253143_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253143_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253151_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253151_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253172_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253172_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253196_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253196_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253197_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253197_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253207_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253207_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253212_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253212_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253220_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253220_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253236_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253236_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253242_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253242_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253243_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253243_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253273_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253273_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253290_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253290_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253291_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253291_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253302_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253302_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253304_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253304_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253306_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253306_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253312_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253312_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253313_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253313_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253326_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253326_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253331_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253331_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 253342_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253342_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253347_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253347_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253356_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253356_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253364_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253364_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253400_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253400_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 253413_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253413_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253458_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253458_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253474_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253474_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253528_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253528_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253530_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253530_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253568_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253568_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253602_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253602_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:40:12.76 +36:18:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253623_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253623_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253626_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253626_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:37:18.74 +40:35:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253627_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253627_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253643_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253643_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:47:15.09 +42:04:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253663_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253663_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253666_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253666_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253671_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253671_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253673_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253673_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253687_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253687_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253693_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253693_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253705_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253705_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253714_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253714_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253718_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253718_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253728_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253728_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253729_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253729_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:10:36.47 +41:28:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253744_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253744_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253760_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253760_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253775_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253775_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:42:55.26 +37:35:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253787_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253787_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253797_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253797_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253804_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253804_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253817_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253817_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:54:18.81 +42:06:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253835_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253835_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:58:37.25 +33:56:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253840_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253840_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253842_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253842_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253890_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253890_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253895_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253895_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253914_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253914_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253917_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253917_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:58:27.97 +40:38:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253937_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253937_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253964_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253964_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:55:20.80 +40:52:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253965_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253965_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:41:19.41 +37:02:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253970_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253970_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253981_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253981_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 253984_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 253984_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:33:21.48 +38:02:44.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)
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Considering the candidate 253987_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 253987_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254002_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254002_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254024_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254024_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254027_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254027_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254030_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254030_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254044_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254044_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254047_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254047_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254071_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254071_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254078_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254078_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254084_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254084_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254089_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254089_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254111_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254111_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254128_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254128_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:01:07.90 +39:15:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254189_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254189_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:27:28.64 +35:23:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254195_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254195_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:47:14.34 +41:48:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254215_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254215_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:29:05.40 +39:02:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254223_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254223_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:42:50.17 +37:29:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254233_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254233_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254240_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254240_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:56:49.69 +42:13:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254241_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254241_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:29:32.62 +33:47:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254243_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254243_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254279_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254279_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:42:45.63 +36:52:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254291_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254291_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:39:05.37 +36:51:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254301_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254301_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:41:29.12 +37:46:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254306_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254306_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:32:29.31 +40:06:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254332_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254332_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:32:54.39 +35:30:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254333_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254333_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:31:28.42 +35:34:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254347_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254347_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254378_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254378_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:58:07.66 +38:56:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254390_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254390_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254394_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254394_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:42:06.17 +36:50:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254448_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254448_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:50:52.29 +39:37:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254455_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254455_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:06:46.60 +39:39:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254465_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254465_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:44:54.14 +33:55:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254472_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254472_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:42:46.46 +37:59:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254494_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254494_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:03:59.83 +39:46:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254499_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254499_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:01:53.17 +40:17:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254502_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254502_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:49:54.61 +34:54:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254504_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254504_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:43:58.09 +41:21:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254522_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254522_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:54:04.39 +37:39:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254525_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254525_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:00:54.58 +41:16:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254555_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254555_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:02:40.21 +38:06:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254566_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254566_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:33:39.14 +39:05:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254578_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254578_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254591_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254591_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:59:27.50 +38:47:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254608_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254608_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:02:27.82 +42:04:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254610_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254610_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254613_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254613_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:34:28.44 +39:24:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254623_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254623_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254630_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254630_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:41:07.83 +34:22:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254632_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254632_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254661_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254661_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:44:49.86 +36:56:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254690_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254690_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254713_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254713_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254731_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254731_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:50:11.52 +35:33:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254752_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254752_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:43:32.04 +38:44:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254783_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254783_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:51:54.89 +33:54:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254785_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254785_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:31:28.83 +34:33:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254790_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254790_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254830_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254830_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:57:22.97 +40:56:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254839_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254839_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254870_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254870_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:53:08.53 +40:33:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254881_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254881_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254886_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254886_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:44:49.52 +35:31:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254888_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254888_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:49:54.46 +37:45:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254907_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254907_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:49:46.99 +41:07:49.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254942_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254942_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254946_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254946_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:50:21.00 +41:53:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254976_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 254976_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 254992_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254992_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:09:23.74 +40:29:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254998_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 254998_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:58:13.59 +38:26:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255030_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255030_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:38:02.67 +39:00:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255041_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255041_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255047_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255047_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255072_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255072_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255082_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255082_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255118_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255118_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 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 255148_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255148_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:50:58.32 +39:32:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255164_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255164_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255223_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255223_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255260_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255282_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255282_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255301_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255301_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255307_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255307_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:55:27.30 +42:00:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255334_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255334_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 255340_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255340_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:41:46.79 +35:55:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255396_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255396_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:55:01.61 +42:15:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255419_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255419_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 255459_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255459_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255485_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255485_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255494_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255494_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:43:03.12 +37:32:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255546_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255546_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255550_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255550_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255613_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255613_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255650_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255650_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:00:00.08 +38:42:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255658_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255658_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:58:15.42 +41:40:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255666_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255666_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255678_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255678_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:30:27.96 +41:53:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255755_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255755_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255821_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 255821_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 255858_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255858_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 255907_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 255907_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256119_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256119_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256122_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256122_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256178_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256178_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256227_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256227_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256236_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 256236_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:59:00.14 +41:56:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256275_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256275_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256285_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256285_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256313_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256313_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256319_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 256319_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:41:51.03 +35:55:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256327_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256327_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256378_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 256378_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:46:08.83 +35:33:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256381_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256381_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256587_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256587_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256603_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 256603_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 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 256646_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256646_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 256750_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 256750_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257101_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257101_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257135_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257135_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257207_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257207_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257346_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257346_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257371_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257371_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257390_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257390_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257439_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257439_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257475_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257475_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257480_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257480_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257605_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257605_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257630_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257630_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257657_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257657_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257667_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 257667_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 22:00:32.81 +39:39:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257748_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257748_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257790_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257790_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257838_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257838_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 257945_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 257945_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 257954_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 257954_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:44:52.63 +41:26:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257965_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 257965_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258002_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258002_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258026_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258026_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258043_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258043_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258050_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 258050_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 258058_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258058_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258112_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258112_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258121_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258121_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258156_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258156_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258196_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258196_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258219_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258219_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258225_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258225_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258228_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258228_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258302_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258302_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258335_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258335_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258364_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258364_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258365_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258365_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258379_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258379_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258403_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258403_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258432_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 258432_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 258440_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258440_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258444_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 258444_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 258473_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258473_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258517_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258517_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258521_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258521_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258531_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258531_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258582_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258582_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258585_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258585_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258599_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258599_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258631_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258631_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258669_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258669_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258699_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258699_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258706_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258706_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258714_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258714_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258774_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 258774_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 258777_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258777_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258793_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258793_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258795_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 258795_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 258797_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258797_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258808_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258808_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258815_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258815_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258852_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258852_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258858_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258858_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258863_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258863_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258872_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258872_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258926_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258926_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258931_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258931_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258933_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258933_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258937_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258937_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258944_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258944_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258966_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258966_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258967_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258967_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 258980_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 258980_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259023_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259023_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 259061_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259061_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 259070_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259070_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259080_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259080_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259124_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259124_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259142_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259142_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 259152_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259152_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259153_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259153_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259157_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259157_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259182_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259182_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259186_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259186_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259187_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259187_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259193_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259193_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259203_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259203_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259241_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259241_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259254_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259254_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259311_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259311_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259319_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259319_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259321_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259321_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259343_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259343_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259357_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259357_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259369_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259369_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259417_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259417_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259418_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259418_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259428_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259428_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 259455_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259455_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259466_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259466_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259478_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259478_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259486_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259486_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259499_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259499_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259504_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259504_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 259505_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259505_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259509_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259509_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259511_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259511_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259519_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259519_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259523_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259523_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259529_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259529_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259545_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259545_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259548_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259548_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259560_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259560_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259616_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259616_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259622_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259622_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259647_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259647_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259702_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259702_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259750_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259750_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259751_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259751_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259761_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259761_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259767_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259767_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259772_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259772_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259795_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259795_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259801_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259801_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259831_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259831_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
**** FOUND 21:28:04.15 +38:59:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259849_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 259849_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 259852_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259852_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259859_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259859_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259872_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259872_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259894_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259894_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259896_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259896_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259926_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259926_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259942_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259942_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259958_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259958_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259963_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259963_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259970_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259970_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259976_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259976_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259977_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259977_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259989_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259989_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 259998_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 259998_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260000_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260000_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260018_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260018_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260040_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260040_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260048_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260048_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260056_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260056_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260074_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260074_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260087_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260087_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260111_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260111_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260143_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260143_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260154_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260154_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260161_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260161_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260170_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260170_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260174_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260174_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260183_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260183_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260187_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260187_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260190_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260190_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260194_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260194_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260216_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260216_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260219_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260219_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260234_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260234_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260238_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260238_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260245_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260245_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260254_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260254_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260266_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260266_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260270_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260270_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260283_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260283_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260291_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260291_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 260293_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260293_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260328_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260328_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260336_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260336_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260342_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260342_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260347_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260347_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260371_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260371_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260377_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260377_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260389_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260389_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260390_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260390_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260393_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260393_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260394_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260394_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260400_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260400_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260408_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260408_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260415_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260415_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260425_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260425_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260433_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260433_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260447_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260447_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260456_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260456_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260460_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260460_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260463_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260463_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260520_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260520_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260522_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260522_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260543_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260543_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260551_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260551_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260553_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260553_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260559_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260559_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260566_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260566_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260581_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260581_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260582_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260582_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260586_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260586_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260587_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260587_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260606_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260606_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260613_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260613_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260621_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260621_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260623_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260623_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260641_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260641_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260642_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260642_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260653_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260653_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260654_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260654_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260679_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260679_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260686_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260686_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260712_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260712_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260729_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260729_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260736_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260736_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260755_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260755_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260779_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260779_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260780_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260780_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260797_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260797_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260818_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260818_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260827_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260827_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260830_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260830_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260831_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260831_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260856_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260856_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260872_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260872_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260880_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260880_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260891_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260891_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260896_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260896_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260897_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260897_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260921_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260921_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 260933_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
The candidate 260933_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382 did not pass the final checks
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Considering the candidate 260962_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 260962_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 261017_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 261017_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 261049_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 261049_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 261053_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 261053_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 261071_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 261071_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 261176_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 261176_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
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Considering the candidate 261245_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
Preparing report for the candidate 261245_fd_Cyg-07-Q2b1x1_2026-05-11_03-10-47_20.00sec_-4.90C_LIGHT_0382
make_report_in_HTML.sh Phase 2 (HTML assembly): 20s
make_report_in_HTML.sh TOTAL: 756s
Prepared the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
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21:45:12.21 +40:36:36.9
21:49:25.05 +42:02:02.8
21:45:58.77 +39:55:46.8
21:50:22.55 +40:29:51.6
21:34:38.98 +38:53:37.6
21:39:22.59 +41:40:38.5
21:40:31.69 +41:13:38.5
21:45:08.22 +34:07:00.6
21:46:37.51 +40:59:09.7
21:51:16.57 +41:52:17.0
21:28:44.78 +40:00:03.1
21:28:54.40 +40:16:40.9
21:37:02.71 +36:17:37.7
21:34:21.84 +35:35:52.5
21:59:29.16 +39:40:32.7
21:34:26.47 +39:32:18.8
21:39:30.80 +37:21:42.4
21:50:42.00 +37:37:59.1
21:46:04.17 +39:02:58.2
21:36:40.49 +40:02:26.4
21:29:56.43 +36:57:31.6
21:37:40.29 +36:45:52.0
21:40:19.70 +35:37:23.5
21:48:39.15 +37:49:35.0
21:54:20.83 +39:10:07.1
21:34:43.80 +39:32:52.7
21:34:30.95 +37:25:09.5
21:45:41.64 +42:01:42.6
21:29:12.22 +35:45:11.1
21:47:00.98 +41:24:09.3
21:49:57.53 +36:11:59.4
21:44:11.75 +40:40:16.9
21:45:54.45 +37:57:42.2
21:40:51.91 +37:15:12.2
21:42:52.72 +36:02:59.3
21:40:55.96 +35:39:12.4
21:44:21.52 +38:41:36.0
21:37:04.90 +35:55:01.1
21:52:31.17 +41:00:05.7
21:30:32.98 +34:04:08.9
21:35:25.02 +37:18:31.0
21:49:21.18 +40:59:12.5
21:44:25.53 +41:41:20.2
21:58:49.47 +40:28:43.1
21:50:07.66 +42:10:52.1
21:43:52.27 +38:47:06.8
21:51:02.72 +40:49:27.0
21:46:33.45 +37:56:10.3
22:00:27.78 +40:13:16.8
21:49:29.08 +36:55:04.2
22:02:20.88 +39:30:33.9
########### Completed Cyg-07-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:37:22.59 +37:20:59.2
21:56:43.79 +40:46:35.1
21:32:46.06 +37:06:20.3
21:39:49.97 +38:35:47.4
21:49:23.73 +39:00:35.9
21:29:18.50 +38:46:45.3
21:35:59.60 +40:25:24.8
21:36:56.47 +36:30:11.3
21:47:21.70 +36:09:48.3
21:38:52.80 +38:18:22.9
21:34:54.35 +35:45:42.5
21:49:05.46 +40:42:33.5
21:37:37.57 +39:15:52.6
21:55:24.97 +39:42:13.4
21:40:39.53 +36:27:53.0
21:57:32.70 +38:48:28.7
21:45:04.66 +40:22:24.7
21:55:46.17 +35:47:05.8
21:31:26.61 +39:18:37.8
21:38:15.65 +36:10:02.1
21:46:11.75 +36:11:01.4
21:40:23.68 +39:00:28.4
21:36:18.88 +36:34:10.5
21:30:30.86 +38:24:14.2
21:41:16.01 +42:07:07.3
21:51:31.73 +37:29:41.7
21:36:44.12 +39:54:03.5
21:31:11.07 +35:03:50.6
21:38:44.15 +35:57:37.8
21:39:43.24 +34:48:32.9
21:27:52.85 +41:24:14.8
21:43:44.31 +34:49:09.2
21:27:27.91 +39:54:37.7
21:50:55.91 +34:03:35.1
21:55:39.57 +36:53:20.5
21:44:37.46 +38:02:16.4
22:08:32.33 +35:58:54.1
21:51:26.68 +38:24:23.9
21:36:58.25 +37:51:36.9
22:06:56.03 +41:38:43.3
21:48:31.20 +41:08:42.7
22:05:37.24 +38:57:41.5
21:38:33.76 +37:39:20.4
21:40:15.50 +37:50:19.7
21:38:51.21 +41:31:56.0
22:00:34.77 +38:25:34.0
21:38:21.00 +42:10:14.8
21:32:45.17 +38:02:04.6
21:40:56.29 +40:31:32.9
21:53:53.72 +40:08:53.0
21:41:28.53 +41:30:43.3
22:10:45.38 +40:14:53.4
21:55:57.22 +40:10:24.0
21:43:23.74 +33:45:12.7
21:38:23.56 +40:06:15.1
22:04:27.90 +38:05:25.5
21:28:22.20 +41:32:01.4
21:35:26.51 +41:08:48.9
21:36:48.40 +35:29:07.4
22:12:11.79 +41:08:45.6
21:43:17.64 +38:29:47.6
21:40:43.77 +37:22:59.4
21:27:41.84 +38:45:45.6
21:36:54.33 +40:36:46.8
21:59:40.16 +41:01:39.7
22:00:33.53 +41:25:45.6
22:01:22.50 +40:55:08.0
21:57:03.95 +40:57:15.4
21:29:00.32 +38:59:30.9
21:26:09.27 +40:15:20.0
21:32:29.76 +41:05:24.6
21:48:47.08 +40:08:12.7
22:02:11.34 +35:32:41.3
21:34:56.24 +40:57:06.9
21:35:35.31 +35:59:25.8
21:40:56.30 +41:13:23.8
21:32:44.34 +41:15:17.7
21:27:24.13 +33:39:56.9
22:05:39.73 +34:53:38.4
21:35:27.08 +41:28:51.2
21:44:09.48 +37:55:02.4
21:33:13.79 +37:12:42.6
21:31:02.18 +37:39:41.2
21:37:46.82 +36:44:34.6
21:32:51.79 +35:15:26.5
22:06:01.50 +39:10:17.5
21:28:09.36 +41:14:35.7
21:30:32.09 +35:46:45.3
22:01:26.27 +38:07:01.4
21:59:06.42 +34:00:16.6
21:36:49.73 +39:45:20.4
21:34:29.38 +39:23:39.0
22:09:13.51 +39:15:45.3
21:27:30.60 +37:13:07.7
21:42:12.49 +38:54:22.8
21:44:26.41 +41:28:26.4
21:39:00.52 +38:41:35.3
21:33:58.53 +36:17:17.2
22:02:42.57 +41:44:10.0
21:54:02.63 +41:59:37.9
21:57:59.28 +41:37:11.8
21:43:12.09 +34:12:51.4
21:48:12.49 +41:41:11.4
21:29:54.96 +37:14:44.7
21:28:25.43 +36:06:45.9
21:36:48.46 +38:51:41.2
21:33:14.96 +33:54:30.5
21:35:57.88 +41:51:55.4
21:27:38.07 +38:16:30.6
22:10:19.98 +38:44:20.3
21:34:43.04 +37:25:55.5
21:26:46.15 +37:00:06.3
22:05:01.96 +41:27:43.6
21:27:39.75 +41:28:18.2
21:37:13.68 +40:19:25.2
21:26:55.28 +38:03:54.4
21:49:15.18 +35:18:20.3
21:59:01.85 +36:26:57.2
21:27:12.39 +39:44:02.8
21:29:34.38 +38:30:18.3
22:02:04.57 +37:45:26.7
21:28:53.79 +35:00:37.1
21:56:00.57 +37:10:55.4
21:29:32.76 +34:41:59.4
22:07:43.39 +37:37:05.2
21:29:00.60 +35:14:16.8
21:56:34.42 +37:00:26.7
21:36:18.34 +40:03:06.5
21:35:21.77 +41:16:18.0
21:30:44.48 +35:40:18.1
21:48:08.00 +39:26:18.2
21:28:41.27 +40:32:26.6
21:26:43.80 +36:22:02.7
21:28:38.45 +34:34:49.6
21:50:34.29 +37:11:01.8
21:47:02.39 +41:50:19.7
21:30:51.93 +34:46:06.8
21:30:59.29 +35:39:20.0
21:28:05.38 +38:26:58.6
21:32:15.23 +37:15:00.3
21:29:37.20 +34:35:10.6
21:56:29.29 +36:52:34.7
21:42:31.34 +35:51:14.4
21:27:07.54 +35:14:55.6
21:26:49.68 +38:35:30.6
21:36:08.49 +35:55:08.0
21:32:35.85 +35:36:09.3
21:39:31.97 +40:39:06.6
21:28:25.12 +39:09:59.0
21:26:44.70 +36:58:52.9
21:57:22.92 +41:48:54.2
21:28:21.49 +39:21:51.2
21:29:38.89 +36:14:26.1
21:34:17.58 +36:20:30.7
21:28:43.67 +35:42:02.8
21:46:36.96 +37:07:18.4
21:40:15.11 +36:00:22.8
21:32:09.67 +40:20:08.4
21:33:29.39 +37:59:53.2
21:31:50.24 +41:32:44.7
22:02:09.53 +41:51:03.0
21:51:39.08 +36:55:29.1
21:28:08.33 +36:20:38.4
21:32:38.88 +34:43:57.6
21:43:05.89 +37:32:43.5
21:46:29.48 +40:15:30.5
21:41:04.96 +34:50:45.4
21:36:03.50 +41:27:53.0
21:26:38.67 +38:32:27.5
21:27:19.93 +35:12:54.6
21:36:10.81 +41:24:44.2
21:31:39.39 +36:46:27.4
21:27:17.19 +38:38:14.0
21:35:57.22 +40:17:36.8
21:28:47.59 +41:03:28.1
21:32:33.19 +38:39:50.3
21:44:32.22 +40:17:32.3
21:34:14.73 +36:36:51.4
21:28:43.52 +36:04:03.0
21:28:44.18 +38:13:29.3
21:35:31.74 +40:47:48.9
21:31:57.29 +36:19:01.8
21:42:45.62 +38:41:53.6
21:42:33.69 +41:45:50.0
21:51:39.57 +40:18:34.1
21:35:10.37 +39:24:30.9
21:28:40.93 +39:00:16.9
21:37:11.01 +41:54:60.0
21:31:07.07 +41:09:16.3
21:31:53.06 +36:06:56.4
21:50:31.71 +38:39:09.1
21:57:10.53 +42:10:40.2
21:46:56.37 +37:17:26.5
21:55:16.04 +41:56:18.7
21:28:33.73 +35:11:45.3
21:38:19.71 +39:47:35.3
21:31:41.34 +38:39:50.7
21:29:50.36 +34:12:18.7
21:36:24.24 +40:56:09.1
21:26:38.83 +39:47:21.9
21:26:51.58 +34:03:09.6
21:28:36.97 +36:44:01.2
21:32:17.26 +41:34:26.1
21:26:38.36 +41:30:09.8
21:43:56.61 +39:49:06.2
21:28:20.86 +36:08:60.0
21:32:16.51 +41:10:13.7
21:33:48.63 +40:09:52.7
21:29:41.64 +39:40:21.7
21:33:24.18 +35:46:28.9
21:32:11.98 +41:33:25.9
21:28:45.01 +38:10:24.9
21:44:55.04 +40:18:07.5
21:28:24.59 +39:10:26.3
21:32:20.07 +33:48:08.4
21:30:16.06 +39:31:30.0
21:31:06.96 +39:46:47.1
21:28:27.96 +35:31:22.4
21:53:00.58 +35:46:12.7
21:34:31.85 +40:00:32.6
21:35:58.37 +39:59:36.1
21:45:57.17 +39:56:06.6
21:43:24.96 +38:44:40.6
21:31:57.16 +41:47:00.4
21:32:40.29 +34:47:34.8
21:47:32.45 +41:45:09.2
21:49:58.72 +41:45:12.8
21:43:28.73 +37:46:48.3
21:41:24.07 +39:05:04.5
21:37:25.90 +37:09:17.1
21:54:32.74 +35:25:30.7
21:42:01.73 +41:13:56.3
21:29:41.34 +41:08:36.9
21:35:51.43 +40:29:40.1
21:48:42.14 +37:37:36.5
21:40:37.29 +42:07:42.5
21:28:21.99 +40:06:48.3
21:36:17.98 +38:04:45.5
21:33:39.97 +33:37:45.1
21:51:40.04 +38:49:49.0
21:46:24.78 +41:13:00.8
21:59:42.19 +41:00:47.0
21:26:49.77 +40:01:27.0
22:01:55.46 +41:18:33.7
21:34:53.21 +38:42:28.1
21:39:45.87 +39:07:09.7
21:51:49.78 +37:26:01.7
21:35:04.43 +35:48:30.7
21:54:13.73 +42:03:13.6
21:33:15.84 +41:05:44.8
21:36:45.81 +37:27:45.6
21:53:17.78 +39:27:52.6
21:43:25.56 +36:45:53.3
21:33:43.13 +37:03:45.9
21:35:22.67 +38:34:23.4
21:30:52.00 +36:48:41.6
21:26:29.45 +38:23:36.6
21:31:04.46 +38:40:10.2
21:26:33.88 +37:40:38.8
21:59:56.14 +38:33:11.3
21:33:02.70 +37:08:25.1
21:42:26.91 +41:38:32.4
21:47:16.33 +40:11:10.3
21:31:06.05 +36:31:15.7
21:45:33.11 +39:44:22.6
21:30:48.43 +33:38:08.4
21:27:45.97 +37:48:40.8
21:43:40.18 +40:38:45.6
21:32:42.44 +36:55:39.2
21:40:59.68 +40:51:38.8
21:41:36.39 +36:01:13.3
21:43:18.85 +42:12:55.3
21:59:55.38 +41:14:21.2
21:32:28.57 +41:35:15.2
21:40:19.51 +35:38:54.4
22:02:22.53 +41:34:46.7
21:47:40.82 +39:31:35.5
21:40:21.14 +39:47:14.2
21:46:33.41 +36:26:40.7
21:39:51.01 +41:51:15.6
21:42:58.43 +36:37:09.6
22:02:54.66 +40:29:56.2
21:40:44.23 +35:27:42.4
21:29:46.84 +38:09:45.8
21:28:45.90 +38:15:12.3
21:33:20.63 +39:12:48.5
21:32:07.67 +37:19:42.8
21:42:46.32 +41:48:21.2
21:49:46.22 +40:24:27.8
21:32:41.24 +35:18:25.0
21:45:06.37 +36:34:15.4
21:43:09.00 +34:51:35.6
21:45:12.21 +40:36:36.9
21:49:25.05 +42:02:02.8
21:45:58.77 +39:55:46.8
21:50:22.55 +40:29:51.6
21:34:38.98 +38:53:37.6
21:39:22.59 +41:40:38.5
21:40:31.69 +41:13:38.5
21:45:08.22 +34:07:00.6
21:46:37.51 +40:59:09.7
21:51:16.57 +41:52:17.0
21:28:44.78 +40:00:03.1
21:28:54.40 +40:16:40.9
21:37:02.71 +36:17:37.7
21:34:21.84 +35:35:52.5
21:59:29.16 +39:40:32.7
21:34:26.47 +39:32:18.8
21:39:30.80 +37:21:42.4
21:50:42.00 +37:37:59.1
21:46:04.17 +39:02:58.2
21:36:40.49 +40:02:26.4
21:29:56.43 +36:57:31.6
21:37:40.29 +36:45:52.0
21:40:19.70 +35:37:23.5
21:48:39.15 +37:49:35.0
21:54:20.83 +39:10:07.1
21:34:43.80 +39:32:52.7
21:34:30.95 +37:25:09.5
21:45:41.64 +42:01:42.6
21:29:12.22 +35:45:11.1
21:47:00.98 +41:24:09.3
21:49:57.53 +36:11:59.4
21:44:11.75 +40:40:16.9
21:45:54.45 +37:57:42.2
21:40:51.91 +37:15:12.2
21:42:52.72 +36:02:59.3
21:40:55.96 +35:39:12.4
21:44:21.52 +38:41:36.0
21:37:04.90 +35:55:01.1
21:52:31.17 +41:00:05.7
21:30:32.98 +34:04:08.9
21:35:25.02 +37:18:31.0
21:49:21.18 +40:59:12.5
21:44:25.53 +41:41:20.2
21:58:49.47 +40:28:43.1
21:50:07.66 +42:10:52.1
21:43:52.27 +38:47:06.8
21:51:02.72 +40:49:27.0
21:46:33.45 +37:56:10.3
22:00:27.78 +40:13:16.8
21:49:29.08 +36:55:04.2
22:02:20.88 +39:30:33.9
###################################################################################
21:37:22.59 +37:20:59.2 -- not an asteroid (will add it to exclusion list)
21:56:43.79 +40:46:35.1 -- not an asteroid (will add it to exclusion list)
21:32:46.06 +37:06:20.3 -- not an asteroid (will add it to exclusion list)
21:39:49.97 +38:35:47.4 -- not an asteroid (will add it to exclusion list)
21:49:23.73 +39:00:35.9 -- not an asteroid (will add it to exclusion list)
21:29:18.50 +38:46:45.3 -- not an asteroid (will add it to exclusion list)
21:35:59.60 +40:25:24.8 -- not an asteroid (will add it to exclusion list)
21:36:56.47 +36:30:11.3 -- not an asteroid (will add it to exclusion list)
21:47:21.70 +36:09:48.3 -- not an asteroid (will add it to exclusion list)
21:38:52.80 +38:18:22.9 -- not an asteroid (will add it to exclusion list)
21:34:54.35 +35:45:42.5 -- not an asteroid (will add it to exclusion list)
21:49:05.46 +40:42:33.5 -- not an asteroid (will add it to exclusion list)
21:37:37.57 +39:15:52.6 -- not an asteroid (will add it to exclusion list)
21:55:24.97 +39:42:13.4 -- not an asteroid (will add it to exclusion list)
21:40:39.53 +36:27:53.0 -- not an asteroid (will add it to exclusion list)
21:57:32.70 +38:48:28.7 -- not an asteroid (will add it to exclusion list)
21:45:04.66 +40:22:24.7 -- not an asteroid (will add it to exclusion list)
21:55:46.17 +35:47:05.8 -- not an asteroid (will add it to exclusion list)
21:31:26.61 +39:18:37.8 -- not an asteroid (will add it to exclusion list)
21:38:15.65 +36:10:02.1 -- not an asteroid (will add it to exclusion list)
21:46:11.75 +36:11:01.4 -- not an asteroid (will add it to exclusion list)
21:40:23.68 +39:00:28.4 -- not an asteroid (will add it to exclusion list)
21:36:18.88 +36:34:10.5 -- not an asteroid (will add it to exclusion list)
21:30:30.86 +38:24:14.2 -- not an asteroid (will add it to exclusion list)
21:41:16.01 +42:07:07.3 -- not an asteroid (will add it to exclusion list)
21:51:31.73 +37:29:41.7 -- not an asteroid (will add it to exclusion list)
21:36:44.12 +39:54:03.5 -- not an asteroid (will add it to exclusion list)
21:31:11.07 +35:03:50.6 -- not an asteroid (will add it to exclusion list)
21:38:44.15 +35:57:37.8 -- not an asteroid (will add it to exclusion list)
21:39:43.24 +34:48:32.9 -- not an asteroid (will add it to exclusion list)
21:27:52.85 +41:24:14.8 -- not an asteroid (will add it to exclusion list)
21:43:44.31 +34:49:09.2 -- not an asteroid (will add it to exclusion list)
21:27:27.91 +39:54:37.7 -- not an asteroid (will add it to exclusion list)
21:50:55.91 +34:03:35.1 -- not an asteroid (will add it to exclusion list)
21:55:39.57 +36:53:20.5 -- not an asteroid (will add it to exclusion list)
21:44:37.46 +38:02:16.4 -- not an asteroid (will add it to exclusion list)
22:08:32.33 +35:58:54.1 -- not an asteroid (will add it to exclusion list)
21:51:26.68 +38:24:23.9 -- not an asteroid (will add it to exclusion list)
21:36:58.25 +37:51:36.9 -- not an asteroid (will add it to exclusion list)
22:06:56.03 +41:38:43.3 -- not an asteroid (will add it to exclusion list)
21:48:31.20 +41:08:42.7 -- not an asteroid (will add it to exclusion list)
22:05:37.24 +38:57:41.5 -- not an asteroid (will add it to exclusion list)
21:38:33.76 +37:39:20.4 -- not an asteroid (will add it to exclusion list)
21:40:15.50 +37:50:19.7 -- not an asteroid (will add it to exclusion list)
21:38:51.21 +41:31:56.0 -- not an asteroid (will add it to exclusion list)
22:00:34.77 +38:25:34.0 -- not an asteroid (will add it to exclusion list)
21:38:21.00 +42:10:14.8 -- not an asteroid (will add it to exclusion list)
21:32:45.17 +38:02:04.6 -- not an asteroid (will add it to exclusion list)
21:40:56.29 +40:31:32.9 -- not an asteroid (will add it to exclusion list)
21:53:53.72 +40:08:53.0 -- not an asteroid (will add it to exclusion list)
21:41:28.53 +41:30:43.3 -- not an asteroid (will add it to exclusion list)
22:10:45.38 +40:14:53.4 -- not an asteroid (will add it to exclusion list)
21:55:57.22 +40:10:24.0 -- not an asteroid (will add it to exclusion list)
21:43:23.74 +33:45:12.7 -- not an asteroid (will add it to exclusion list)
21:38:23.56 +40:06:15.1 -- not an asteroid (will add it to exclusion list)
22:04:27.90 +38:05:25.5 -- not an asteroid (will add it to exclusion list)
21:28:22.20 +41:32:01.4 -- not an asteroid (will add it to exclusion list)
21:35:26.51 +41:08:48.9 -- not an asteroid (will add it to exclusion list)
21:36:48.40 +35:29:07.4 -- not an asteroid (will add it to exclusion list)
22:12:11.79 +41:08:45.6 -- not an asteroid (will add it to exclusion list)
21:43:17.64 +38:29:47.6 -- not an asteroid (will add it to exclusion list)
21:40:43.77 +37:22:59.4 -- not an asteroid (will add it to exclusion list)
21:27:41.84 +38:45:45.6 -- not an asteroid (will add it to exclusion list)
21:36:54.33 +40:36:46.8 -- not an asteroid (will add it to exclusion list)
21:59:40.16 +41:01:39.7 -- not an asteroid (will add it to exclusion list)
22:00:33.53 +41:25:45.6 -- not an asteroid (will add it to exclusion list)
22:01:22.50 +40:55:08.0 -- not an asteroid (will add it to exclusion list)
21:57:03.95 +40:57:15.4 -- not an asteroid (will add it to exclusion list)
21:29:00.32 +38:59:30.9 -- not an asteroid (will add it to exclusion list)
21:26:09.27 +40:15:20.0 -- not an asteroid (will add it to exclusion list)
21:32:29.76 +41:05:24.6 -- not an asteroid (will add it to exclusion list)
21:48:47.08 +40:08:12.7 -- not an asteroid (will add it to exclusion list)
22:02:11.34 +35:32:41.3 -- not an asteroid (will add it to exclusion list)
21:34:56.24 +40:57:06.9 -- not an asteroid (will add it to exclusion list)
21:35:35.31 +35:59:25.8 -- not an asteroid (will add it to exclusion list)
21:40:56.30 +41:13:23.8 -- not an asteroid (will add it to exclusion list)
21:32:44.34 +41:15:17.7 -- not an asteroid (will add it to exclusion list)
21:27:24.13 +33:39:56.9 -- not an asteroid (will add it to exclusion list)
22:05:39.73 +34:53:38.4 -- not an asteroid (will add it to exclusion list)
21:35:27.08 +41:28:51.2 -- not an asteroid (will add it to exclusion list)
21:44:09.48 +37:55:02.4 -- not an asteroid (will add it to exclusion list)
21:33:13.79 +37:12:42.6 -- not an asteroid (will add it to exclusion list)
21:31:02.18 +37:39:41.2 -- not an asteroid (will add it to exclusion list)
21:37:46.82 +36:44:34.6 -- not an asteroid (will add it to exclusion list)
21:32:51.79 +35:15:26.5 -- not an asteroid (will add it to exclusion list)
22:06:01.50 +39:10:17.5 -- not an asteroid (will add it to exclusion list)
21:28:09.36 +41:14:35.7 -- not an asteroid (will add it to exclusion list)
21:30:32.09 +35:46:45.3 -- not an asteroid (will add it to exclusion list)
22:01:26.27 +38:07:01.4 -- not an asteroid (will add it to exclusion list)
21:59:06.42 +34:00:16.6 -- not an asteroid (will add it to exclusion list)
21:36:49.73 +39:45:20.4 -- not an asteroid (will add it to exclusion list)
21:34:29.38 +39:23:39.0 -- not an asteroid (will add it to exclusion list)
22:09:13.51 +39:15:45.3 -- not an asteroid (will add it to exclusion list)
21:27:30.60 +37:13:07.7 -- not an asteroid (will add it to exclusion list)
21:42:12.49 +38:54:22.8 -- not an asteroid (will add it to exclusion list)
21:44:26.41 +41:28:26.4 -- not an asteroid (will add it to exclusion list)
21:39:00.52 +38:41:35.3 -- not an asteroid (will add it to exclusion list)
21:33:58.53 +36:17:17.2 -- not an asteroid (will add it to exclusion list)
22:02:42.57 +41:44:10.0 -- not an asteroid (will add it to exclusion list)
21:54:02.63 +41:59:37.9 -- not an asteroid (will add it to exclusion list)
21:57:59.28 +41:37:11.8 -- not an asteroid (will add it to exclusion list)
21:43:12.09 +34:12:51.4 -- not an asteroid (will add it to exclusion list)
21:48:12.49 +41:41:11.4 -- not an asteroid (will add it to exclusion list)
21:29:54.96 +37:14:44.7 -- not an asteroid (will add it to exclusion list)
21:28:25.43 +36:06:45.9 -- not an asteroid (will add it to exclusion list)
21:36:48.46 +38:51:41.2 -- not an asteroid (will add it to exclusion list)
21:33:14.96 +33:54:30.5 -- not an asteroid (will add it to exclusion list)
21:35:57.88 +41:51:55.4 -- not an asteroid (will add it to exclusion list)
21:27:38.07 +38:16:30.6 -- not an asteroid (will add it to exclusion list)
22:10:19.98 +38:44:20.3 -- not an asteroid (will add it to exclusion list)
21:34:43.04 +37:25:55.5 -- not an asteroid (will add it to exclusion list)
21:26:46.15 +37:00:06.3 -- not an asteroid (will add it to exclusion list)
22:05:01.96 +41:27:43.6 -- not an asteroid (will add it to exclusion list)
21:27:39.75 +41:28:18.2 -- not an asteroid (will add it to exclusion list)
21:37:13.68 +40:19:25.2 -- not an asteroid (will add it to exclusion list)
21:26:55.28 +38:03:54.4 -- not an asteroid (will add it to exclusion list)
21:49:15.18 +35:18:20.3 -- not an asteroid (will add it to exclusion list)
21:59:01.85 +36:26:57.2 -- not an asteroid (will add it to exclusion list)
21:27:12.39 +39:44:02.8 -- not an asteroid (will add it to exclusion list)
21:29:34.38 +38:30:18.3 -- not an asteroid (will add it to exclusion list)
22:02:04.57 +37:45:26.7 -- not an asteroid (will add it to exclusion list)
21:28:53.79 +35:00:37.1 -- not an asteroid (will add it to exclusion list)
21:56:00.57 +37:10:55.4 -- not an asteroid (will add it to exclusion list)
21:29:32.76 +34:41:59.4 -- not an asteroid (will add it to exclusion list)
22:07:43.39 +37:37:05.2 -- not an asteroid (will add it to exclusion list)
21:29:00.60 +35:14:16.8 -- not an asteroid (will add it to exclusion list)
21:56:34.42 +37:00:26.7 -- not an asteroid (will add it to exclusion list)
21:36:18.34 +40:03:06.5 -- not an asteroid (will add it to exclusion list)
21:35:21.77 +41:16:18.0 -- not an asteroid (will add it to exclusion list)
21:30:44.48 +35:40:18.1 -- not an asteroid (will add it to exclusion list)
21:48:08.00 +39:26:18.2 -- not an asteroid (will add it to exclusion list)
21:28:41.27 +40:32:26.6 -- not an asteroid (will add it to exclusion list)
21:26:43.80 +36:22:02.7 -- not an asteroid (will add it to exclusion list)
21:28:38.45 +34:34:49.6 -- not an asteroid (will add it to exclusion list)
21:50:34.29 +37:11:01.8 -- not an asteroid (will add it to exclusion list)
21:47:02.39 +41:50:19.7 -- not an asteroid (will add it to exclusion list)
21:30:51.93 +34:46:06.8 -- not an asteroid (will add it to exclusion list)
21:30:59.29 +35:39:20.0 -- not an asteroid (will add it to exclusion list)
21:28:05.38 +38:26:58.6 -- not an asteroid (will add it to exclusion list)
21:32:15.23 +37:15:00.3 -- not an asteroid (will add it to exclusion list)
21:29:37.20 +34:35:10.6 -- not an asteroid (will add it to exclusion list)
21:56:29.29 +36:52:34.7 -- not an asteroid (will add it to exclusion list)
21:42:31.34 +35:51:14.4 -- not an asteroid (will add it to exclusion list)
21:27:07.54 +35:14:55.6 -- not an asteroid (will add it to exclusion list)
21:26:49.68 +38:35:30.6 -- not an asteroid (will add it to exclusion list)
21:36:08.49 +35:55:08.0 -- not an asteroid (will add it to exclusion list)
21:32:35.85 +35:36:09.3 -- not an asteroid (will add it to exclusion list)
21:39:31.97 +40:39:06.6 -- not an asteroid (will add it to exclusion list)
21:28:25.12 +39:09:59.0 -- not an asteroid (will add it to exclusion list)
21:26:44.70 +36:58:52.9 -- not an asteroid (will add it to exclusion list)
21:57:22.92 +41:48:54.2 -- not an asteroid (will add it to exclusion list)
21:28:21.49 +39:21:51.2 -- not an asteroid (will add it to exclusion list)
21:29:38.89 +36:14:26.1 -- not an asteroid (will add it to exclusion list)
21:34:17.58 +36:20:30.7 -- not an asteroid (will add it to exclusion list)
21:28:43.67 +35:42:02.8 -- not an asteroid (will add it to exclusion list)
21:46:36.96 +37:07:18.4 -- not an asteroid (will add it to exclusion list)
21:40:15.11 +36:00:22.8 -- not an asteroid (will add it to exclusion list)
21:32:09.67 +40:20:08.4 -- not an asteroid (will add it to exclusion list)
21:33:29.39 +37:59:53.2 -- not an asteroid (will add it to exclusion list)
21:31:50.24 +41:32:44.7 -- not an asteroid (will add it to exclusion list)
22:02:09.53 +41:51:03.0 -- not an asteroid (will add it to exclusion list)
21:51:39.08 +36:55:29.1 -- not an asteroid (will add it to exclusion list)
21:28:08.33 +36:20:38.4 -- not an asteroid (will add it to exclusion list)
21:32:38.88 +34:43:57.6 -- not an asteroid (will add it to exclusion list)
21:43:05.89 +37:32:43.5 -- not an asteroid (will add it to exclusion list)
21:46:29.48 +40:15:30.5 -- not an asteroid (will add it to exclusion list)
21:41:04.96 +34:50:45.4 -- not an asteroid (will add it to exclusion list)
21:36:03.50 +41:27:53.0 -- not an asteroid (will add it to exclusion list)
21:26:38.67 +38:32:27.5 -- not an asteroid (will add it to exclusion list)
21:27:19.93 +35:12:54.6 -- not an asteroid (will add it to exclusion list)
21:36:10.81 +41:24:44.2 -- not an asteroid (will add it to exclusion list)
21:31:39.39 +36:46:27.4 -- not an asteroid (will add it to exclusion list)
21:27:17.19 +38:38:14.0 -- not an asteroid (will add it to exclusion list)
21:35:57.22 +40:17:36.8 -- not an asteroid (will add it to exclusion list)
21:28:47.59 +41:03:28.1 -- not an asteroid (will add it to exclusion list)
21:32:33.19 +38:39:50.3 -- not an asteroid (will add it to exclusion list)
21:44:32.22 +40:17:32.3 -- not an asteroid (will add it to exclusion list)
21:34:14.73 +36:36:51.4 -- not an asteroid (will add it to exclusion list)
21:28:43.52 +36:04:03.0 -- not an asteroid (will add it to exclusion list)
21:28:44.18 +38:13:29.3 -- not an asteroid (will add it to exclusion list)
21:35:31.74 +40:47:48.9 -- not an asteroid (will add it to exclusion list)
21:31:57.29 +36:19:01.8 -- not an asteroid (will add it to exclusion list)
21:42:45.62 +38:41:53.6 -- not an asteroid (will add it to exclusion list)
21:42:33.69 +41:45:50.0 -- not an asteroid (will add it to exclusion list)
21:51:39.57 +40:18:34.1 -- not an asteroid (will add it to exclusion list)
21:35:10.37 +39:24:30.9 -- not an asteroid (will add it to exclusion list)
21:28:40.93 +39:00:16.9 -- not an asteroid (will add it to exclusion list)
21:37:11.01 +41:54:60.0 -- not an asteroid (will add it to exclusion list)
21:31:07.07 +41:09:16.3 -- not an asteroid (will add it to exclusion list)
21:31:53.06 +36:06:56.4 -- not an asteroid (will add it to exclusion list)
21:50:31.71 +38:39:09.1 -- not an asteroid (will add it to exclusion list)
21:57:10.53 +42:10:40.2 -- not an asteroid (will add it to exclusion list)
21:46:56.37 +37:17:26.5 -- not an asteroid (will add it to exclusion list)
21:55:16.04 +41:56:18.7 -- not an asteroid (will add it to exclusion list)
21:28:33.73 +35:11:45.3 -- not an asteroid (will add it to exclusion list)
21:38:19.71 +39:47:35.3 -- not an asteroid (will add it to exclusion list)
21:31:41.34 +38:39:50.7 -- not an asteroid (will add it to exclusion list)
21:29:50.36 +34:12:18.7 -- not an asteroid (will add it to exclusion list)
21:36:24.24 +40:56:09.1 -- not an asteroid (will add it to exclusion list)
21:26:38.83 +39:47:21.9 -- not an asteroid (will add it to exclusion list)
21:26:51.58 +34:03:09.6 -- not an asteroid (will add it to exclusion list)
21:28:36.97 +36:44:01.2 -- not an asteroid (will add it to exclusion list)
21:32:17.26 +41:34:26.1 -- not an asteroid (will add it to exclusion list)
21:26:38.36 +41:30:09.8 -- not an asteroid (will add it to exclusion list)
21:43:56.61 +39:49:06.2 -- not an asteroid (will add it to exclusion list)
21:28:20.86 +36:08:60.0 -- not an asteroid (will add it to exclusion list)
21:32:16.51 +41:10:13.7 -- not an asteroid (will add it to exclusion list)
21:33:48.63 +40:09:52.7 -- not an asteroid (will add it to exclusion list)
21:29:41.64 +39:40:21.7 -- not an asteroid (will add it to exclusion list)
21:33:24.18 +35:46:28.9 -- not an asteroid (will add it to exclusion list)
21:32:11.98 +41:33:25.9 -- not an asteroid (will add it to exclusion list)
21:28:45.01 +38:10:24.9 -- not an asteroid (will add it to exclusion list)
21:44:55.04 +40:18:07.5 -- not an asteroid (will add it to exclusion list)
21:28:24.59 +39:10:26.3 -- not an asteroid (will add it to exclusion list)
21:32:20.07 +33:48:08.4 -- not an asteroid (will add it to exclusion list)
21:30:16.06 +39:31:30.0 -- not an asteroid (will add it to exclusion list)
21:31:06.96 +39:46:47.1 -- not an asteroid (will add it to exclusion list)
21:28:27.96 +35:31:22.4 -- not an asteroid (will add it to exclusion list)
21:53:00.58 +35:46:12.7 -- not an asteroid (will add it to exclusion list)
21:34:31.85 +40:00:32.6 -- not an asteroid (will add it to exclusion list)
21:35:58.37 +39:59:36.1 -- not an asteroid (will add it to exclusion list)
21:45:57.17 +39:56:06.6 -- not an asteroid (will add it to exclusion list)
21:43:24.96 +38:44:40.6 -- not an asteroid (will add it to exclusion list)
21:31:57.16 +41:47:00.4 -- not an asteroid (will add it to exclusion list)
21:32:40.29 +34:47:34.8 -- not an asteroid (will add it to exclusion list)
21:47:32.45 +41:45:09.2 -- not an asteroid (will add it to exclusion list)
21:49:58.72 +41:45:12.8 -- not an asteroid (will add it to exclusion list)
21:43:28.73 +37:46:48.3 -- not an asteroid (will add it to exclusion list)
21:41:24.07 +39:05:04.5 -- not an asteroid (will add it to exclusion list)
21:37:25.90 +37:09:17.1 -- not an asteroid (will add it to exclusion list)
21:54:32.74 +35:25:30.7 -- not an asteroid (will add it to exclusion list)
21:42:01.73 +41:13:56.3 -- not an asteroid (will add it to exclusion list)
21:29:41.34 +41:08:36.9 -- not an asteroid (will add it to exclusion list)
21:35:51.43 +40:29:40.1 -- not an asteroid (will add it to exclusion list)
21:48:42.14 +37:37:36.5 -- not an asteroid (will add it to exclusion list)
21:40:37.29 +42:07:42.5 -- not an asteroid (will add it to exclusion list)
21:28:21.99 +40:06:48.3 -- not an asteroid (will add it to exclusion list)
21:36:17.98 +38:04:45.5 -- not an asteroid (will add it to exclusion list)
21:33:39.97 +33:37:45.1 -- not an asteroid (will add it to exclusion list)
21:51:40.04 +38:49:49.0 -- not an asteroid (will add it to exclusion list)
21:46:24.78 +41:13:00.8 -- not an asteroid (will add it to exclusion list)
21:59:42.19 +41:00:47.0 -- not an asteroid (will add it to exclusion list)
21:26:49.77 +40:01:27.0 -- not an asteroid (will add it to exclusion list)
22:01:55.46 +41:18:33.7 -- not an asteroid (will add it to exclusion list)
21:34:53.21 +38:42:28.1 -- not an asteroid (will add it to exclusion list)
21:39:45.87 +39:07:09.7 -- not an asteroid (will add it to exclusion list)
21:51:49.78 +37:26:01.7 -- not an asteroid (will add it to exclusion list)
21:35:04.43 +35:48:30.7 -- not an asteroid (will add it to exclusion list)
21:54:13.73 +42:03:13.6 -- not an asteroid (will add it to exclusion list)
21:33:15.84 +41:05:44.8 -- not an asteroid (will add it to exclusion list)
21:36:45.81 +37:27:45.6 -- not an asteroid (will add it to exclusion list)
21:53:17.78 +39:27:52.6 -- not an asteroid (will add it to exclusion list)
21:43:25.56 +36:45:53.3 -- not an asteroid (will add it to exclusion list)
21:33:43.13 +37:03:45.9 -- not an asteroid (will add it to exclusion list)
21:35:22.67 +38:34:23.4 -- not an asteroid (will add it to exclusion list)
21:30:52.00 +36:48:41.6 -- not an asteroid (will add it to exclusion list)
21:26:29.45 +38:23:36.6 -- not an asteroid (will add it to exclusion list)
21:31:04.46 +38:40:10.2 -- not an asteroid (will add it to exclusion list)
21:26:33.88 +37:40:38.8 -- not an asteroid (will add it to exclusion list)
21:59:56.14 +38:33:11.3 -- not an asteroid (will add it to exclusion list)
21:33:02.70 +37:08:25.1 -- not an asteroid (will add it to exclusion list)
21:42:26.91 +41:38:32.4 -- not an asteroid (will add it to exclusion list)
21:47:16.33 +40:11:10.3 -- not an asteroid (will add it to exclusion list)
21:31:06.05 +36:31:15.7 -- not an asteroid (will add it to exclusion list)
21:45:33.11 +39:44:22.6 -- not an asteroid (will add it to exclusion list)
21:30:48.43 +33:38:08.4 -- not an asteroid (will add it to exclusion list)
21:27:45.97 +37:48:40.8 -- not an asteroid (will add it to exclusion list)
21:43:40.18 +40:38:45.6 -- not an asteroid (will add it to exclusion list)
21:32:42.44 +36:55:39.2 -- not an asteroid (will add it to exclusion list)
21:40:59.68 +40:51:38.8 -- not an asteroid (will add it to exclusion list)
21:41:36.39 +36:01:13.3 -- not an asteroid (will add it to exclusion list)
21:43:18.85 +42:12:55.3 -- not an asteroid (will add it to exclusion list)
21:59:55.38 +41:14:21.2 -- not an asteroid (will add it to exclusion list)
21:32:28.57 +41:35:15.2 -- not an asteroid (will add it to exclusion list)
21:40:19.51 +35:38:54.4 -- not an asteroid (will add it to exclusion list)
22:02:22.53 +41:34:46.7 -- not an asteroid (will add it to exclusion list)
21:47:40.82 +39:31:35.5 -- not an asteroid (will add it to exclusion list)
21:40:21.14 +39:47:14.2 -- not an asteroid (will add it to exclusion list)
21:46:33.41 +36:26:40.7 -- not an asteroid (will add it to exclusion list)
21:39:51.01 +41:51:15.6 -- not an asteroid (will add it to exclusion list)
21:42:58.43 +36:37:09.6 -- not an asteroid (will add it to exclusion list)
22:02:54.66 +40:29:56.2 -- not an asteroid (will add it to exclusion list)
21:40:44.23 +35:27:42.4 -- not an asteroid (will add it to exclusion list)
21:29:46.84 +38:09:45.8 -- not an asteroid (will add it to exclusion list)
21:28:45.90 +38:15:12.3 -- not an asteroid (will add it to exclusion list)
21:33:20.63 +39:12:48.5 -- not an asteroid (will add it to exclusion list)
21:32:07.67 +37:19:42.8 -- not an asteroid (will add it to exclusion list)
21:42:46.32 +41:48:21.2 -- not an asteroid (will add it to exclusion list)
21:49:46.22 +40:24:27.8 -- not an asteroid (will add it to exclusion list)
21:32:41.24 +35:18:25.0 -- not an asteroid (will add it to exclusion list)
21:45:06.37 +36:34:15.4 -- not an asteroid (will add it to exclusion list)
21:43:09.00 +34:51:35.6 -- not an asteroid (will add it to exclusion list)
21:45:12.21 +40:36:36.9 -- not an asteroid (will add it to exclusion list)
21:49:25.05 +42:02:02.8 -- not an asteroid (will add it to exclusion list)
21:45:58.77 +39:55:46.8 -- not an asteroid (will add it to exclusion list)
21:50:22.55 +40:29:51.6 -- not an asteroid (will add it to exclusion list)
21:34:38.98 +38:53:37.6 -- not an asteroid (will add it to exclusion list)
21:39:22.59 +41:40:38.5 -- not an asteroid (will add it to exclusion list)
21:40:31.69 +41:13:38.5 -- not an asteroid (will add it to exclusion list)
21:45:08.22 +34:07:00.6 -- not an asteroid (will add it to exclusion list)
21:46:37.51 +40:59:09.7 -- not an asteroid (will add it to exclusion list)
21:51:16.57 +41:52:17.0 -- not an asteroid (will add it to exclusion list)
21:28:44.78 +40:00:03.1 -- not an asteroid (will add it to exclusion list)
21:28:54.40 +40:16:40.9 -- not an asteroid (will add it to exclusion list)
21:37:02.71 +36:17:37.7 -- not an asteroid (will add it to exclusion list)
21:34:21.84 +35:35:52.5 -- not an asteroid (will add it to exclusion list)
21:59:29.16 +39:40:32.7 -- not an asteroid (will add it to exclusion list)
21:34:26.47 +39:32:18.8 -- not an asteroid (will add it to exclusion list)
21:39:30.80 +37:21:42.4 -- not an asteroid (will add it to exclusion list)
21:50:42.00 +37:37:59.1 -- not an asteroid (will add it to exclusion list)
21:46:04.17 +39:02:58.2 -- not an asteroid (will add it to exclusion list)
21:36:40.49 +40:02:26.4 -- not an asteroid (will add it to exclusion list)
21:29:56.43 +36:57:31.6 -- not an asteroid (will add it to exclusion list)
21:37:40.29 +36:45:52.0 -- not an asteroid (will add it to exclusion list)
21:40:19.70 +35:37:23.5 -- not an asteroid (will add it to exclusion list)
21:48:39.15 +37:49:35.0 -- not an asteroid (will add it to exclusion list)
21:54:20.83 +39:10:07.1 -- not an asteroid (will add it to exclusion list)
21:34:43.80 +39:32:52.7 -- not an asteroid (will add it to exclusion list)
21:34:30.95 +37:25:09.5 -- not an asteroid (will add it to exclusion list)
21:45:41.64 +42:01:42.6 -- not an asteroid (will add it to exclusion list)
21:29:12.22 +35:45:11.1 -- not an asteroid (will add it to exclusion list)
21:47:00.98 +41:24:09.3 -- not an asteroid (will add it to exclusion list)
21:49:57.53 +36:11:59.4 -- not an asteroid (will add it to exclusion list)
21:44:11.75 +40:40:16.9 -- not an asteroid (will add it to exclusion list)
21:45:54.45 +37:57:42.2 -- not an asteroid (will add it to exclusion list)
21:40:51.91 +37:15:12.2 -- not an asteroid (will add it to exclusion list)
21:42:52.72 +36:02:59.3 -- not an asteroid (will add it to exclusion list)
21:40:55.96 +35:39:12.4 -- not an asteroid (will add it to exclusion list)
21:44:21.52 +38:41:36.0 -- not an asteroid (will add it to exclusion list)
21:37:04.90 +35:55:01.1 -- not an asteroid (will add it to exclusion list)
21:52:31.17 +41:00:05.7 -- not an asteroid (will add it to exclusion list)
21:30:32.98 +34:04:08.9 -- not an asteroid (will add it to exclusion list)
21:35:25.02 +37:18:31.0 -- not an asteroid (will add it to exclusion list)
21:49:21.18 +40:59:12.5 -- not an asteroid (will add it to exclusion list)
21:44:25.53 +41:41:20.2 -- not an asteroid (will add it to exclusion list)
21:58:49.47 +40:28:43.1 -- not an asteroid (will add it to exclusion list)
21:50:07.66 +42:10:52.1 -- not an asteroid (will add it to exclusion list)
21:43:52.27 +38:47:06.8 -- not an asteroid (will add it to exclusion list)
21:51:02.72 +40:49:27.0 -- not an asteroid (will add it to exclusion list)
21:46:33.45 +37:56:10.3 -- not an asteroid (will add it to exclusion list)
22:00:27.78 +40:13:16.8 -- not an asteroid (will add it to exclusion list)
21:49:29.08 +36:55:04.2 -- not an asteroid (will add it to exclusion list)
22:02:20.88 +39:30:33.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:26:09.27 +40:15:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:29.45 +38:23:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:33.88 +37:40:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:38.36 +41:30:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:38.67 +38:32:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:38.83 +39:47:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:43.80 +36:22:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:44.70 +36:58:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:46.15 +37:00:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:49.68 +38:35:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:49.77 +40:01:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:51.58 +34:03:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:55.28 +38:03:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:07.54 +35:14:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:12.39 +39:44:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:17.19 +38:38:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:19.93 +35:12:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:24.13 +33:39:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:27.91 +39:54:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:30.60 +37:13:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:38.07 +38:16:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:39.75 +41:28:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:41.84 +38:45:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:45.97 +37:48:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:52.85 +41:24:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:05.38 +38:26:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:08.33 +36:20:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:09.36 +41:14:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:20.86 +36:08:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:21.49 +39:21:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:21.99 +40:06:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:22.20 +41:32:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:24.59 +39:10:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:25.12 +39:09:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:25.43 +36:06:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:27.96 +35:31:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:33.73 +35:11:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:36.97 +36:44:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:38.45 +34:34:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:40.93 +39:00:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:41.27 +40:32:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.52 +36:04:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:43.67 +35:42:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:44.18 +38:13:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:44.78 +40:00:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:45.01 +38:10:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:45.90 +38:15:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:47.59 +41:03:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:53.79 +35:00:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:54.40 +40:16:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.32 +38:59:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:00.60 +35:14:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:12.22 +35:45:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:18.50 +38:46:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:32.76 +34:41:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:34.38 +38:30:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:37.20 +34:35:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:38.89 +36:14:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:41.34 +41:08:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:41.64 +39:40:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:46.84 +38:09:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:50.36 +34:12:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:54.96 +37:14:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:56.43 +36:57:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:16.06 +39:31:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:30.86 +38:24:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:32.09 +35:46:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:32.98 +34:04:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:44.48 +35:40:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:48.43 +33:38:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:51.93 +34:46:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:52.00 +36:48:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:59.29 +35:39:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:02.18 +37:39:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:04.46 +38:40:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:06.05 +36:31:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:06.96 +39:46:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:07.07 +41:09:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:11.07 +35:03:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:26.61 +39:18:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:39.39 +36:46:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:41.34 +38:39:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:50.24 +41:32:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:53.06 +36:06:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:57.16 +41:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:57.29 +36:19:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:07.67 +37:19:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:09.67 +40:20:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:11.98 +41:33:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:15.23 +37:15:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:16.51 +41:10:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:17.26 +41:34:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:20.07 +33:48:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:28.57 +41:35:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:29.76 +41:05:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:33.19 +38:39:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:35.85 +35:36:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:38.88 +34:43:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:40.29 +34:47:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:41.24 +35:18:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:42.44 +36:55:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:44.34 +41:15:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:45.17 +38:02:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:46.06 +37:06:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:51.79 +35:15:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:02.70 +37:08:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:13.79 +37:12:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:14.96 +33:54:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:15.84 +41:05:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:20.63 +39:12:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:24.18 +35:46:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:29.39 +37:59:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:39.97 +33:37:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:43.13 +37:03:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:48.63 +40:09:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:58.53 +36:17:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:14.73 +36:36:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:17.58 +36:20:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:21.84 +35:35:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:26.47 +39:32:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:29.38 +39:23:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:30.95 +37:25:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:31.85 +40:00:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:38.98 +38:53:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:43.04 +37:25:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:43.80 +39:32:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:53.21 +38:42:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:54.35 +35:45:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:56.24 +40:57:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:04.43 +35:48:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:10.37 +39:24:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:21.77 +41:16:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:22.67 +38:34:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:25.02 +37:18:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:26.51 +41:08:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:27.08 +41:28:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:31.74 +40:47:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:35.31 +35:59:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:51.43 +40:29:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:57.22 +40:17:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:57.88 +41:51:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:58.37 +39:59:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:59.60 +40:25:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:03.50 +41:27:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:08.49 +35:55:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:10.81 +41:24:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:17.98 +38:04:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:18.34 +40:03:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:18.88 +36:34:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:24.24 +40:56:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:40.49 +40:02:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:44.12 +39:54:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:45.81 +37:27:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:48.40 +35:29:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:48.46 +38:51:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:49.73 +39:45:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:54.33 +40:36:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:56.47 +36:30:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:58.25 +37:51:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:02.71 +36:17:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:04.90 +35:55:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:11.01 +41:54:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:13.68 +40:19:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:22.59 +37:20:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:25.90 +37:09:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:37.57 +39:15:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:40.29 +36:45:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.82 +36:44:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:15.65 +36:10:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:19.71 +39:47:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:21.00 +42:10:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:23.56 +40:06:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:33.76 +37:39:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:44.15 +35:57:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:51.21 +41:31:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:52.80 +38:18:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:00.52 +38:41:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:22.59 +41:40:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:30.80 +37:21:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:31.97 +40:39:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:43.24 +34:48:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:45.87 +39:07:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:49.97 +38:35:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:51.01 +41:51:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:15.11 +36:00:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:15.50 +37:50:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:19.51 +35:38:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:19.70 +35:37:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:21.14 +39:47:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:23.68 +39:00:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:31.69 +41:13:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:37.29 +42:07:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:39.53 +36:27:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.77 +37:22:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:44.23 +35:27:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:51.91 +37:15:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:55.96 +35:39:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.29 +40:31:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:56.30 +41:13:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:59.68 +40:51:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:04.96 +34:50:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:16.01 +42:07:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:24.07 +39:05:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:28.53 +41:30:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:36.39 +36:01:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:01.73 +41:13:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:12.49 +38:54:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:26.91 +41:38:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:31.34 +35:51:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:33.69 +41:45:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:45.62 +38:41:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:46.32 +41:48:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:52.72 +36:02:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:58.43 +36:37:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:05.89 +37:32:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:09.00 +34:51:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:12.09 +34:12:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:17.64 +38:29:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:18.85 +42:12:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:23.74 +33:45:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:24.96 +38:44:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:25.56 +36:45:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:28.73 +37:46:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:40.18 +40:38:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:44.31 +34:49:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:52.27 +38:47:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:56.61 +39:49:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:09.48 +37:55:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:11.75 +40:40:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:21.52 +38:41:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:25.53 +41:41:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:26.41 +41:28:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:32.22 +40:17:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:37.46 +38:02:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:55.04 +40:18:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:04.66 +40:22:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:06.37 +36:34:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:08.22 +34:07:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:12.21 +40:36:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:33.11 +39:44:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:41.64 +42:01:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:54.45 +37:57:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:57.17 +39:56:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:58.77 +39:55:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:04.17 +39:02:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:11.75 +36:11:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:24.78 +41:13:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:29.48 +40:15:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:33.41 +36:26:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:33.45 +37:56:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:36.96 +37:07:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:37.51 +40:59:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:56.37 +37:17:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:00.98 +41:24:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:02.39 +41:50:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:16.33 +40:11:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:21.70 +36:09:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:32.45 +41:45:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:40.82 +39:31:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:08.00 +39:26:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:12.49 +41:41:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:31.20 +41:08:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:39.15 +37:49:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:42.14 +37:37:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:47.08 +40:08:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:05.46 +40:42:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:15.18 +35:18:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:21.18 +40:59:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:23.73 +39:00:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:25.05 +42:02:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:29.08 +36:55:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:46.22 +40:24:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:57.53 +36:11:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:58.72 +41:45:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:07.66 +42:10:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:22.55 +40:29:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:31.71 +38:39:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:34.29 +37:11:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:42.00 +37:37:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:50:55.91 +34:03:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:02.72 +40:49:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:16.57 +41:52:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:26.68 +38:24:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:31.73 +37:29:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.08 +36:55:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:39.57 +40:18:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:40.04 +38:49:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:49.78 +37:26:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:31.17 +41:00:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:00.58 +35:46:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:17.78 +39:27:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:53.72 +40:08:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:02.63 +41:59:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:13.73 +42:03:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:20.83 +39:10:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:32.74 +35:25:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:16.04 +41:56:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:24.97 +39:42:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:39.57 +36:53:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:46.17 +35:47:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:57.22 +40:10:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:00.57 +37:10:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:29.29 +36:52:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:34.42 +37:00:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:43.79 +40:46:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:03.95 +40:57:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:10.53 +42:10:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:22.92 +41:48:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:32.70 +38:48:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:59.28 +41:37:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:49.47 +40:28:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:01.85 +36:26:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:06.42 +34:00:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:29.16 +39:40:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:40.16 +41:01:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:42.19 +41:00:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:55.38 +41:14:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:56.14 +38:33:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:27.78 +40:13:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:33.53 +41:25:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:34.77 +38:25:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:22.50 +40:55:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:26.27 +38:07:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:55.46 +41:18:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:04.57 +37:45:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:09.53 +41:51:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:11.34 +35:32:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:20.88 +39:30:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.53 +41:34:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.57 +41:44:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:54.66 +40:29:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:27.90 +38:05:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:01.96 +41:27:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:37.24 +38:57:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:39.73 +34:53:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:01.50 +39:10:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:56.03 +41:38:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:43.39 +37:37:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:32.33 +35:58:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:13.51 +39:15:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:19.98 +38:44:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:10:45.38 +40:14:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:11.79 +41:08:45.6 -- 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)
21:26:09.27 +40:15:20.0 -- not a known variable star
21:26:29.45 +38:23:36.6 -- a known variable star
21:26:33.88 +37:40:38.8 -- not a known variable star
21:26:38.36 +41:30:09.8 -- a known variable star
21:26:38.67 +38:32:27.5 -- not a known variable star
21:26:38.83 +39:47:21.9 -- not a known variable star
21:26:43.80 +36:22:02.7 -- not a known variable star
21:26:44.70 +36:58:52.9 -- not a known variable star
21:26:46.15 +37:00:06.3 -- not a known variable star
21:26:49.68 +38:35:30.6 -- not a known variable star
21:26:49.77 +40:01:27.0 -- not a known variable star
21:26:51.58 +34:03:09.6 -- a known variable star
21:26:55.28 +38:03:54.4 -- not a known variable star
21:27:07.54 +35:14:55.6 -- not a known variable star
21:27:12.39 +39:44:02.8 -- not a known variable star
21:27:17.19 +38:38:14.0 -- not a known variable star
21:27:19.93 +35:12:54.6 -- not a known variable star
21:27:24.13 +33:39:56.9 -- not a known variable star
21:27:27.91 +39:54:37.7 -- not a known variable star
21:27:30.60 +37:13:07.7 -- not a known variable star
21:27:38.07 +38:16:30.6 -- not a known variable star
21:27:39.75 +41:28:18.2 -- not a known variable star
21:27:41.84 +38:45:45.6 -- not a known variable star
21:27:45.97 +37:48:40.8 -- not a known variable star
21:27:52.85 +41:24:14.8 -- a known variable star
21:28:05.38 +38:26:58.6 -- not a known variable star
21:28:08.33 +36:20:38.4 -- not a known variable star
21:28:09.36 +41:14:35.7 -- not a known variable star
21:28:20.86 +36:08:60.0 -- not a known variable star
21:28:21.49 +39:21:51.2 -- a known variable star
21:28:21.99 +40:06:48.3 -- not a known variable star
21:28:22.20 +41:32:01.4 -- not a known variable star
21:28:24.59 +39:10:26.3 -- not a known variable star
21:28:25.12 +39:09:59.0 -- not a known variable star
21:28:25.43 +36:06:45.9 -- not a known variable star
21:28:27.96 +35:31:22.4 -- not a known variable star
21:28:33.73 +35:11:45.3 -- not a known variable star
21:28:36.97 +36:44:01.2 -- not a known variable star
21:28:38.45 +34:34:49.6 -- not a known variable star
21:28:40.93 +39:00:16.9 -- not a known variable star
21:28:41.27 +40:32:26.6 -- not a known variable star
21:28:43.52 +36:04:03.0 -- not a known variable star
21:28:43.67 +35:42:02.8 -- not a known variable star
21:28:44.18 +38:13:29.3 -- not a known variable star
21:28:44.78 +40:00:03.1 -- not a known variable star
21:28:45.01 +38:10:24.9 -- not a known variable star
21:28:45.90 +38:15:12.3 -- not a known variable star
21:28:47.59 +41:03:28.1 -- not a known variable star
21:28:53.79 +35:00:37.1 -- not a known variable star
21:28:54.40 +40:16:40.9 -- not a known variable star
21:29:00.32 +38:59:30.9 -- not a known variable star
21:29:00.60 +35:14:16.8 -- not a known variable star
21:29:12.22 +35:45:11.1 -- not a known variable star
21:29:18.50 +38:46:45.3 -- not a known variable star
21:29:32.76 +34:41:59.4 -- not a known variable star
21:29:34.38 +38:30:18.3 -- not a known variable star
21:29:37.20 +34:35:10.6 -- a known variable star
21:29:38.89 +36:14:26.1 -- not a known variable star
21:29:41.34 +41:08:36.9 -- not a known variable star
21:29:41.64 +39:40:21.7 -- not a known variable star
21:29:46.84 +38:09:45.8 -- not a known variable star
21:29:50.36 +34:12:18.7 -- not a known variable star
21:29:54.96 +37:14:44.7 -- not a known variable star
21:29:56.43 +36:57:31.6 -- a known variable star
21:30:16.06 +39:31:30.0 -- not a known variable star
21:30:30.86 +38:24:14.2 -- not a known variable star
21:30:32.09 +35:46:45.3 -- not a known variable star
21:30:32.98 +34:04:08.9 -- not a known variable star
21:30:44.48 +35:40:18.1 -- not a known variable star
21:30:48.43 +33:38:08.4 -- not a known variable star
21:30:51.93 +34:46:06.8 -- not a known variable star
21:30:52.00 +36:48:41.6 -- a known variable star
21:30:59.29 +35:39:20.0 -- not a known variable star
21:31:02.18 +37:39:41.2 -- not a known variable star
21:31:04.46 +38:40:10.2 -- not a known variable star
21:31:06.05 +36:31:15.7 -- not a known variable star
21:31:06.96 +39:46:47.1 -- not a known variable star
21:31:07.07 +41:09:16.3 -- not a known variable star
21:31:11.07 +35:03:50.6 -- not a known variable star
21:31:26.61 +39:18:37.8 -- a known variable star
21:31:39.39 +36:46:27.4 -- not a known variable star
21:31:41.34 +38:39:50.7 -- not a known variable star
21:31:50.24 +41:32:44.7 -- not a known variable star
21:31:53.06 +36:06:56.4 -- not a known variable star
21:31:57.16 +41:47:00.4 -- a known variable star
21:31:57.29 +36:19:01.8 -- not a known variable star
21:32:07.67 +37:19:42.8 -- not a known variable star
21:32:09.67 +40:20:08.4 -- not a known variable star
21:32:11.98 +41:33:25.9 -- not a known variable star
21:32:15.23 +37:15:00.3 -- a known variable star
21:32:16.51 +41:10:13.7 -- a known variable star
21:32:17.26 +41:34:26.1 -- not a known variable star
21:32:20.07 +33:48:08.4 -- not a known variable star
21:32:28.57 +41:35:15.2 -- not a known variable star
21:32:29.76 +41:05:24.6 -- not a known variable star
21:32:33.19 +38:39:50.3 -- not a known variable star
21:32:35.85 +35:36:09.3 -- not a known variable star
21:32:38.88 +34:43:57.6 -- not a known variable star
21:32:40.29 +34:47:34.8 -- not a known variable star
21:32:41.24 +35:18:25.0 -- not a known variable star
21:32:42.44 +36:55:39.2 -- not a known variable star
21:32:44.34 +41:15:17.7 -- a known variable star
21:32:45.17 +38:02:04.6 -- not a known variable star
21:32:46.06 +37:06:20.3 -- not a known variable star
21:32:51.79 +35:15:26.5 -- not a known variable star
21:33:02.70 +37:08:25.1 -- not a known variable star
21:33:13.79 +37:12:42.6 -- not a known variable star
21:33:14.96 +33:54:30.5 -- not a known variable star
21:33:15.84 +41:05:44.8 -- not a known variable star
21:33:20.63 +39:12:48.5 -- not a known variable star
21:33:24.18 +35:46:28.9 -- not a known variable star
21:33:29.39 +37:59:53.2 -- a known variable star
21:33:39.97 +33:37:45.1 -- not a known variable star
21:33:43.13 +37:03:45.9 -- not a known variable star
21:33:48.63 +40:09:52.7 -- not a known variable star
21:33:58.53 +36:17:17.2 -- not a known variable star
21:34:14.73 +36:36:51.4 -- not a known variable star
21:34:17.58 +36:20:30.7 -- not a known variable star
21:34:21.84 +35:35:52.5 -- not a known variable star
21:34:26.47 +39:32:18.8 -- a known variable star
21:34:29.38 +39:23:39.0 -- not a known variable star
21:34:30.95 +37:25:09.5 -- a known variable star
21:34:31.85 +40:00:32.6 -- not a known variable star
21:34:38.98 +38:53:37.6 -- not a known variable star
21:34:43.04 +37:25:55.5 -- not a known variable star
21:34:43.80 +39:32:52.7 -- a known variable star
21:34:53.21 +38:42:28.1 -- not a known variable star
21:34:54.35 +35:45:42.5 -- not a known variable star
21:34:56.24 +40:57:06.9 -- a known variable star
21:35:04.43 +35:48:30.7 -- a known variable star
21:35:10.37 +39:24:30.9 -- not a known variable star
21:35:21.77 +41:16:18.0 -- not a known variable star
21:35:22.67 +38:34:23.4 -- not a known variable star
21:35:25.02 +37:18:31.0 -- not a known variable star
21:35:26.51 +41:08:48.9 -- not a known variable star
21:35:27.08 +41:28:51.2 -- not a known variable star
21:35:31.74 +40:47:48.9 -- not a known variable star
21:35:35.31 +35:59:25.8 -- not a known variable star
21:35:51.43 +40:29:40.1 -- a known variable star
21:35:57.22 +40:17:36.8 -- not a known variable star
21:35:57.88 +41:51:55.4 -- a known variable star
21:35:58.37 +39:59:36.1 -- not a known variable star
21:35:59.60 +40:25:24.8 -- not a known variable star
21:36:03.50 +41:27:53.0 -- not a known variable star
21:36:08.49 +35:55:08.0 -- not a known variable star
21:36:10.81 +41:24:44.2 -- not a known variable star
21:36:17.98 +38:04:45.5 -- not a known variable star
21:36:18.34 +40:03:06.5 -- not a known variable star
21:36:18.88 +36:34:10.5 -- not a known variable star
21:36:24.24 +40:56:09.1 -- not a known variable star
21:36:40.49 +40:02:26.4 -- not a known variable star
21:36:44.12 +39:54:03.5 -- not a known variable star
21:36:45.81 +37:27:45.6 -- not a known variable star
21:36:48.40 +35:29:07.4 -- not a known variable star
21:36:48.46 +38:51:41.2 -- not a known variable star
21:36:49.73 +39:45:20.4 -- not a known variable star
21:36:54.33 +40:36:46.8 -- not a known variable star
21:36:56.47 +36:30:11.3 -- a known variable star
21:36:58.25 +37:51:36.9 -- not a known variable star
21:37:02.71 +36:17:37.7 -- not a known variable star
21:37:04.90 +35:55:01.1 -- not a known variable star
21:37:11.01 +41:54:60.0 -- not a known variable star
21:37:13.68 +40:19:25.2 -- not a known variable star
21:37:22.59 +37:20:59.2 -- not a known variable star
21:37:25.90 +37:09:17.1 -- not a known variable star
21:37:37.57 +39:15:52.6 -- a known variable star
21:37:40.29 +36:45:52.0 -- not a known variable star
21:37:46.82 +36:44:34.6 -- a known variable star
21:38:15.65 +36:10:02.1 -- not a known variable star
21:38:19.71 +39:47:35.3 -- not a known variable star
21:38:21.00 +42:10:14.8 -- not a known variable star
21:38:23.56 +40:06:15.1 -- not a known variable star
21:38:33.76 +37:39:20.4 -- not a known variable star
21:38:44.15 +35:57:37.8 -- a known variable star
21:38:51.21 +41:31:56.0 -- a known variable star
21:38:52.80 +38:18:22.9 -- not a known variable star
21:39:00.52 +38:41:35.3 -- not a known variable star
21:39:22.59 +41:40:38.5 -- not a known variable star
21:39:30.80 +37:21:42.4 -- not a known variable star
21:39:31.97 +40:39:06.6 -- not a known variable star
21:39:43.24 +34:48:32.9 -- not a known variable star
21:39:45.87 +39:07:09.7 -- not a known variable star
21:39:49.97 +38:35:47.4 -- not a known variable star
21:39:51.01 +41:51:15.6 -- not a known variable star
21:40:15.11 +36:00:22.8 -- not a known variable star
21:40:15.50 +37:50:19.7 -- not a known variable star
21:40:19.51 +35:38:54.4 -- not a known variable star
21:40:19.70 +35:37:23.5 -- a known variable star
21:40:21.14 +39:47:14.2 -- not a known variable star
21:40:23.68 +39:00:28.4 -- not a known variable star
21:40:31.69 +41:13:38.5 -- not a known variable star
21:40:37.29 +42:07:42.5 -- not a known variable star
21:40:39.53 +36:27:53.0 -- a known variable star
21:40:43.77 +37:22:59.4 -- not a known variable star
21:40:44.23 +35:27:42.4 -- not a known variable star
21:40:51.91 +37:15:12.2 -- not a known variable star
21:40:55.96 +35:39:12.4 -- not a known variable star
21:40:56.29 +40:31:32.9 -- not a known variable star
21:40:56.30 +41:13:23.8 -- not a known variable star
21:40:59.68 +40:51:38.8 -- a known variable star
21:41:04.96 +34:50:45.4 -- not a known variable star
21:41:16.01 +42:07:07.3 -- not a known variable star
21:41:24.07 +39:05:04.5 -- not a known variable star
21:41:28.53 +41:30:43.3 -- not a known variable star
21:41:36.39 +36:01:13.3 -- not a known variable star
21:42:01.73 +41:13:56.3 -- not a known variable star
21:42:12.49 +38:54:22.8 -- a known variable star
21:42:26.91 +41:38:32.4 -- not a known variable star
21:42:31.34 +35:51:14.4 -- not a known variable star
21:42:33.69 +41:45:50.0 -- not a known variable star
21:42:45.62 +38:41:53.6 -- not a known variable star
21:42:46.32 +41:48:21.2 -- not a known variable star
21:42:52.72 +36:02:59.3 -- not a known variable star
21:42:58.43 +36:37:09.6 -- a known variable star
21:43:05.89 +37:32:43.5 -- not a known variable star
21:43:09.00 +34:51:35.6 -- a known variable star
21:43:12.09 +34:12:51.4 -- not a known variable star
21:43:17.64 +38:29:47.6 -- not a known variable star
21:43:18.85 +42:12:55.3 -- not a known variable star
21:43:23.74 +33:45:12.7 -- not a known variable star
21:43:24.96 +38:44:40.6 -- not a known variable star
21:43:25.56 +36:45:53.3 -- not a known variable star
21:43:28.73 +37:46:48.3 -- a known variable star
21:43:40.18 +40:38:45.6 -- not a known variable star
21:43:44.31 +34:49:09.2 -- not a known variable star
21:43:52.27 +38:47:06.8 -- not a known variable star
21:43:56.61 +39:49:06.2 -- not a known variable star
21:44:09.48 +37:55:02.4 -- not a known variable star
21:44:11.75 +40:40:16.9 -- not a known variable star
21:44:21.52 +38:41:36.0 -- not a known variable star
21:44:25.53 +41:41:20.2 -- not a known variable star
21:44:26.41 +41:28:26.4 -- not a known variable star
21:44:32.22 +40:17:32.3 -- not a known variable star
21:44:37.46 +38:02:16.4 -- not a known variable star
21:44:55.04 +40:18:07.5 -- not a known variable star
21:45:04.66 +40:22:24.7 -- not a known variable star
21:45:06.37 +36:34:15.4 -- not a known variable star
21:45:08.22 +34:07:00.6 -- not a known variable star
21:45:12.21 +40:36:36.9 -- not a known variable star
21:45:33.11 +39:44:22.6 -- not a known variable star
21:45:41.64 +42:01:42.6 -- not a known variable star
21:45:54.45 +37:57:42.2 -- not a known variable star
21:45:57.17 +39:56:06.6 -- not a known variable star
21:45:58.77 +39:55:46.8 -- a known variable star
21:46:04.17 +39:02:58.2 -- not a known variable star
21:46:11.75 +36:11:01.4 -- not a known variable star
21:46:24.78 +41:13:00.8 -- a known variable star
21:46:29.48 +40:15:30.5 -- not a known variable star
21:46:33.41 +36:26:40.7 -- not a known variable star
21:46:33.45 +37:56:10.3 -- not a known variable star
21:46:36.96 +37:07:18.4 -- not a known variable star
21:46:37.51 +40:59:09.7 -- not a known variable star
21:46:56.37 +37:17:26.5 -- not a known variable star
21:47:00.98 +41:24:09.3 -- not a known variable star
21:47:02.39 +41:50:19.7 -- a known variable star
21:47:16.33 +40:11:10.3 -- not a known variable star
21:47:21.70 +36:09:48.3 -- not a known variable star
21:47:32.45 +41:45:09.2 -- not a known variable star
21:47:40.82 +39:31:35.5 -- not a known variable star
21:48:08.00 +39:26:18.2 -- not a known variable star
21:48:12.49 +41:41:11.4 -- not a known variable star
21:48:31.20 +41:08:42.7 -- not a known variable star
21:48:39.15 +37:49:35.0 -- not a known variable star
21:48:42.14 +37:37:36.5 -- a known variable star
21:48:47.08 +40:08:12.7 -- not a known variable star
21:49:05.46 +40:42:33.5 -- not a known variable star
21:49:15.18 +35:18:20.3 -- not a known variable star
21:49:21.18 +40:59:12.5 -- not a known variable star
21:49:23.73 +39:00:35.9 -- not a known variable star
21:49:25.05 +42:02:02.8 -- not a known variable star
21:49:29.08 +36:55:04.2 -- not a known variable star
21:49:46.22 +40:24:27.8 -- not a known variable star
21:49:57.53 +36:11:59.4 -- not a known variable star
21:49:58.72 +41:45:12.8 -- not a known variable star
21:50:07.66 +42:10:52.1 -- not a known variable star
21:50:22.55 +40:29:51.6 -- not a known variable star
21:50:31.71 +38:39:09.1 -- not a known variable star
21:50:34.29 +37:11:01.8 -- not a known variable star
21:50:42.00 +37:37:59.1 -- not a known variable star
21:50:55.91 +34:03:35.1 -- not a known variable star
21:51:02.72 +40:49:27.0 -- a known variable star
21:51:16.57 +41:52:17.0 -- not a known variable star
21:51:26.68 +38:24:23.9 -- not a known variable star
21:51:31.73 +37:29:41.7 -- not a known variable star
21:51:39.08 +36:55:29.1 -- not a known variable star
21:51:39.57 +40:18:34.1 -- not a known variable star
21:51:40.04 +38:49:49.0 -- not a known variable star
21:51:49.78 +37:26:01.7 -- a known variable star
21:52:31.17 +41:00:05.7 -- not a known variable star
21:53:00.58 +35:46:12.7 -- not a known variable star
21:53:17.78 +39:27:52.6 -- not a known variable star
21:53:53.72 +40:08:53.0 -- not a known variable star
21:54:02.63 +41:59:37.9 -- not a known variable star
21:54:13.73 +42:03:13.6 -- not a known variable star
21:54:20.83 +39:10:07.1 -- not a known variable star
21:54:32.74 +35:25:30.7 -- not a known variable star
21:55:16.04 +41:56:18.7 -- not a known variable star
21:55:24.97 +39:42:13.4 -- not a known variable star
21:55:39.57 +36:53:20.5 -- not a known variable star
21:55:46.17 +35:47:05.8 -- not a known variable star
21:55:57.22 +40:10:24.0 -- not a known variable star
21:56:00.57 +37:10:55.4 -- not a known variable star
21:56:29.29 +36:52:34.7 -- not a known variable star
21:56:34.42 +37:00:26.7 -- not a known variable star
21:56:43.79 +40:46:35.1 -- not a known variable star
21:57:03.95 +40:57:15.4 -- not a known variable star
21:57:10.53 +42:10:40.2 -- not a known variable star
21:57:22.92 +41:48:54.2 -- not a known variable star
21:57:32.70 +38:48:28.7 -- not a known variable star
21:57:59.28 +41:37:11.8 -- not a known variable star
21:58:49.47 +40:28:43.1 -- not a known variable star
21:59:01.85 +36:26:57.2 -- not a known variable star
21:59:06.42 +34:00:16.6 -- not a known variable star
21:59:29.16 +39:40:32.7 -- not a known variable star
21:59:40.16 +41:01:39.7 -- not a known variable star
21:59:42.19 +41:00:47.0 -- not a known variable star
21:59:55.38 +41:14:21.2 -- not a known variable star
21:59:56.14 +38:33:11.3 -- a known variable star
22:00:27.78 +40:13:16.8 -- not a known variable star
22:00:33.53 +41:25:45.6 -- not a known variable star
22:00:34.77 +38:25:34.0 -- not a known variable star
22:01:22.50 +40:55:08.0 -- not a known variable star
22:01:26.27 +38:07:01.4 -- not a known variable star
22:01:55.46 +41:18:33.7 -- not a known variable star
22:02:04.57 +37:45:26.7 -- not a known variable star
22:02:09.53 +41:51:03.0 -- not a known variable star
22:02:11.34 +35:32:41.3 -- not a known variable star
22:02:20.88 +39:30:33.9 -- not a known variable star
22:02:22.53 +41:34:46.7 -- not a known variable star
22:02:42.57 +41:44:10.0 -- not a known variable star
22:02:54.66 +40:29:56.2 -- not a known variable star
22:04:27.90 +38:05:25.5 -- not a known variable star
22:05:01.96 +41:27:43.6 -- not a known variable star
22:05:37.24 +38:57:41.5 -- not a known variable star
22:05:39.73 +34:53:38.4 -- a known variable star
22:06:01.50 +39:10:17.5 -- not a known variable star
22:06:56.03 +41:38:43.3 -- not a known variable star
22:07:43.39 +37:37:05.2 -- not a known variable star
22:08:32.33 +35:58:54.1 -- not a known variable star
22:09:13.51 +39:15:45.3 -- not a known variable star
22:10:19.98 +38:44:20.3 -- a known variable star
22:10:45.38 +40:14:53.4 -- not a known variable star
22:12:11.79 +41:08:45.6 -- a known variable star
Found 300 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
343 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 343 (excluding asteroids and hot pixels, 300 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)2461171.84045278 -observatory V36
02:56:11.97 +16:19:55.4 Mercury (-1.9mag)
05:17:46.13 +24:24:34.5 Venus (-3.9mag)
01:29:40.39 +08:30:54.6 Mars (1.2mag)
07:27:10.79 +22:19:33.5 Jupiter (-2.0mag)
00:39:51.62 +01:54:06.6 Saturn (0.9mag)
03:53:28.12 +20:05:30.3 Uranus (5.8mag)
00:13:50.83 +00:03:16.9 Neptune (7.8mag)
20:34:14.04 -22:56:03.8 Pluto (14.5mag)
22:39:24.38 -09:07:37.5 Moon (-9.9mag)
-rw-r--r-- 1 apache apache 362 May 11 03:41 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461171.84045278:
07:27:18.69 +22:19:14.0 Io (5.9mag)
07:27:21.26 +22:19:08.8 Europa (6.1mag)
07:26:57.10 +22:20:11.1 Ganymede (5.5mag)
07:26:39.36 +22:20:48.9 Callisto (6.7mag)
07:29:10.07 +21:58:12.4 Himalia (15.5mag)
07:27:10.82 +22:19:35.3 Thebe (16.4mag)
07:29:38.22 +22:25:07.6 Elara (17.4mag)
07:27:44.44 +22:46:14.8 Pasiphae (17.6mag)
07:34:49.27 +22:19:29.3 Carme (18.7mag)
00:39:58.69 +01:53:50.1 Titan (8.7mag)
00:39:53.32 +01:54:20.6 Rhea (10.0mag)
00:39:39.70 +01:52:09.4 Iapetus (11.4mag)
00:39:44.82 +01:54:34.2 Hyperion (14.7mag)
00:41:05.35 +01:59:53.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 11 03:41 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461171.84045278:
16:57:38.30 -29:16:02.1 JWST
18:08:34.14 +32:51:52.8 Chandra
19:31:52.64 +05:02:24.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 11 03:41 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461171.84045278 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
07:41:53.64 +25:50:22.1 17.7mag P/2009 WX51 (Catalina)
18:55:29.61 -30:29:55.4 13.7mag P/2010 H2 (Vales)
05:27:14.64 -68:39:20.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:39:21.04 +31:38:57.2 17.4mag C/2017 K2 (PANSTARRS)
17:25:02.97 +13:17:43.6 17.7mag C/2021 G2 (ATLAS)
23:14:34.84 +30:21:27.6 17.2mag C/2022 E2 (ATLAS)
04:59:42.24 +26:37:41.3 16.3mag C/2022 N2 (PANSTARRS)
09:12:36.23 +31:50:21.5 16.4mag C/2022 QE78 (ATLAS)
08:37:48.66 +02:10:51.4 17.5mag C/2022 R6 (PANSTARRS)
18:44:25.55 +20:25:35.6 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:30:47.11 -11:10:11.5 17.5mag P/2023 B1 (PANSTARRS)
09:00:23.39 -08:18:10.0 17.9mag C/2023 F3 (ATLAS)
22:12:34.55 +64:35:44.0 17.6mag C/2023 H5 (Lemmon)
18:46:32.67 -04:33:52.0 13.8mag C/2023 R1 (PANSTARRS)
16:10:02.56 +88:09:38.9 17.9mag C/2023 X2 (Lemmon)
06:36:56.32 +63:38:13.7 17.4mag C/2024 A1 (ATLAS)
06:01:56.63 +24:21:44.3 12.5mag C/2024 E1 (Wierzchos)
16:00:17.21 +10:18:34.2 17.3mag C/2024 G6 (ATLAS)
20:23:19.70 +22:36:48.1 14.3mag C/2024 J3 (ATLAS)
03:50:16.74 -18:53:40.6 16.2mag C/2024 T5 (ATLAS)
05:39:37.73 +39:39:38.9 17.8mag C/2025 J1 (Borisov)
12:12:01.80 +53:08:34.5 16.3mag C/2025 L1 (ATLAS)
05:35:44.60 -07:44:53.2 10.3mag C/2025 R3 (PANSTARRS)
12:44:27.87 +04:14:55.5 17.3mag C/2025 Y1 (ATLAS)
05:26:04.40 +01:22:33.3 17.8mag C/2026 A1 (MAPS)
01:04:26.59 +40:53:43.0 15.3mag C/2026 B2 (Sun-Gao)
19:31:44.07 -08:25:41.0 10.3mag 10P/Tempel
14:29:05.25 -00:11:42.4 16.3mag 24P/Schaumasse
10:59:02.56 -00:56:45.8 15.8mag 29P/Schwassmann-Wachmann
10:43:01.63 -02:44:42.9 17.4mag 43P/Wolf-Harrington
02:28:12.57 +21:36:57.4 17.4mag 47P/Ashbrook-Jackson
08:00:59.95 +31:11:00.6 16.9mag 63P/Wild
23:59:18.86 -08:39:52.9 15.7mag 65P/Gunn
05:15:36.07 +28:40:18.0 16.2mag 76P/West-Kohoutek-Ikemura
02:03:03.48 +12:57:42.0 14.1mag 78P/Gehrels
00:14:12.68 -02:03:57.2 15.0mag 88P/Howell
03:25:51.99 +26:31:29.4 15.1mag 93P/Lovas
05:46:37.33 +33:14:20.7 15.9mag 123P/West-Hartley
09:03:52.53 +26:49:52.4 16.3mag 124P/Mrkos
03:13:23.58 +16:59:24.7 16.4mag 128P/Shoemaker-Holt
03:37:50.39 +17:11:05.8 17.6mag 131P/Mueller
03:42:50.38 +19:07:17.4 11.4mag 141P/Machholz
03:47:08.85 +13:18:52.1 11.3mag 141P-A/Machholz
02:27:25.91 +09:30:09.5 10.6mag 141P-D/Machholz
02:36:57.35 -29:14:14.0 17.8mag 161P/Hartley-IRAS
02:14:52.24 +11:12:03.1 14.9mag 162P/SidingSpring
17:12:17.74 -10:51:32.9 16.1mag 235P/LINEAR
06:31:04.97 +35:51:27.8 17.1mag 240P/NEAT
07:54:20.54 -02:54:37.1 18.0mag 242P/Spahr
23:20:39.15 -13:13:34.2 17.2mag 260P/McNaught
02:53:42.12 +26:37:43.7 17.8mag 295P/LINEAR
15:30:02.42 +08:12:22.1 17.4mag 391P/Kowalski
07:47:10.42 +21:15:42.7 17.8mag 450P/LONEOS
06:14:49.29 +43:31:51.2 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 11 03:41 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
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
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
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
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
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
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
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 2026-04-9.29 13.32
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
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
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
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
-rw-r--r-- 1 apache apache 5.8K May 11 03:41 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
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
-rw-r--r-- 1 apache apache 188K May 11 03:41 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:01:59.740 +52:36:43.30 AT 2026liv 2026-04-11.86 22.12
14:34:20.990 +44:20:22.25 AT 2026liu 2026-04-05.77 20.59
14:02:10.870 +41:47:18.26 AT 2026lit 2026-03-29.87 20.68
13:04:54.460 +03:49:27.58 AT 2026lis 2026-05-02.63 19.49
14:08:47.670 +05:29:34.68 AT 2026lir 2026-04-20.75 22.4
10:52:38.850 +04:28:22.81 AT 2026liq 2026-04-16.58 22.12
09:17:17.861 +24:52:59.16 AT 2026lip 2026-05-04.29 19.167
18:43:35.838 -18:26:46.49 AT 2026lio 2026-04-29.46 17.465
19:45:06.300 +04:59:48.72 AT 2026lin 2026-05-02.45 18.394
18:13:26.628 +10:07:10.12 AT 2026lim 2026-05-01.46 19.503
09:21:14.008 -20:11:51.31 AT 2026lil 2026-04-08.38 20.07
19:39:56.943 +09:19:03.51 AT 2026lik 2026-04-30.43 18.527
19:36:07.718 -13:37:37.69 AT 2026lij 2026-04-30.42 18.198
19:43:59.404 +10:35:29.56 AT 2026lii 2026-04-29.43 19.494
17:53:28.438 -13:50:29.84 AT 2026lih 2026-04-29.42 17.636
14:26:40.200 -24:48:39.30 AT 2026lig 2026-05-04.25 14.7
09:37:27.727 +05:56:37.23 AT 2026lif 2026-05-03.87 19.246
11:03:06.682 +17:02:24.06 AT 2026lie 2026-05-03.89 19.67
10:50:39.250 +31:29:59.62 AT 2026lid 2026-05-01.88 19.34
11:59:09.620 +30:06:03.09 AT 2026lic 2026-05-03.91 19.53
-rw-r--r-- 1 apache apache 30K May 11 03:41 tns_transients_list.txt
