This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207496127841632768,2461153.6902,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207496127841632768 20260423.1902 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AC Aur,2461153.6902,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AC Aur 20260423.1902 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 12.69 06:24:03.79 +44:40:33.8
169.67234 14.19296 galactic Aur Second-epoch detections are separated by 3.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:24:03.79 +44:40:33.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:24:03.79 +44:40:33.8: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:24:03.79 +44:40:33.8: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 12.69CV 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 04 23.1902 2461153.6902 12.29 05:18:04.61 +44:13:03.0
164.19030 3.74319 galactic Aur 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 | 05:18:04.61 +44:13:03.0 (user input) | T | P | (position from user input) J-Ks=0.560+/-0.036 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:04.61 +44:13:03.0: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:04.61 +44:13:03.0: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.09 05:20:12.06 +41:50:45.1
166.36082 2.70437 galactic Aur 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 | target | 05:20:12.06 +41:50:45.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.405+/-0.030 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:12.06 +41:50:45.1: 14.17 +/- 0.21 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:12.06 +41:50:45.1: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.16 05:22:38.68 +42:27:33.6
166.11234 3.42541 galactic Aur Second-epoch detections are separated by 0.4" and 6.8 pix
The object was found in VSX 1" Gaia DR3 195233476517200256
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.280 G 13.310 G B
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:38.68 +42:27:33.6: 13.59 +/- 0.15 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:38.68 +42:27:33.6: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 195233476517200256,2461153.6902,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195233476517200256 20260423.1902 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 04 23.1902 2461153.6902 12.53 06:16:43.96 +44:42:40.5
169.07589 13.02577 galactic Aur 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 | 06:16:43.96 +44:42:40.5 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.028 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:16:43.96 +44:42:40.5: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:16:43.96 +44:42:40.5: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 12.05 05:20:53.49 +43:20:16.7
165.20457 3.65819 galactic Aur Second-epoch detections are separated by 2.2" and 6.7 pix
The object was found in VSX 1" Gaia DR3 207390162408467072
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.330 G 13.360 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:53.49 +43:20:16.7: 13.36 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:53.49 +43:20:16.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 207390162408467072,2461153.6902,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207390162408467072 20260423.1902 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 04 23.1902 2461153.6902 12.32 06:08:41.39 +41:19:36.9
171.50413 10.20504 galactic Aur Second-epoch detections are separated by 6.7" and 7.9 pix
The object was found in VSX13" ZTF J060840.88+411949.0
Type: SR
# Max. Min./Amp. JD0 Period
14.870 r Y 0.066 r 2458398.29200 42.986541000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:08:41.39 +41:19:36.9: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:08:41.39 +41:19:36.9: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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
ZTF J060840.88+411949.0,2461153.6902,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J060840.88+411949.0 20260423.1902 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 04 23.1902 2461153.6902 11.96 05:16:32.32 +43:44:08.9
164.42514 3.23954 galactic Aur 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 J079.1445+43.7357 | 05:16:32.32 +43:44:08.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:16:32.32 +43:44:08.9: 13.90 +/- 0.18 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:16:32.32 +43:44:08.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 J079.1445+43.7357,2461153.6902,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.1445+43.7357 20260423.1902 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 04 23.1902 2461153.6902 11.76 05:18:33.91 +42:17:09.8
165.82549 2.70731 galactic Aur Second-epoch detections are separated by 1.5" and 6.7 pix
The object was found in VSX20" ZTF J051833.80+421730.2
Type: BY
# Max. Min./Amp. JD0 Period
18.673 r Y 0.125 r 2458435.86390 0.920697000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:33.91 +42:17:09.8: 14.49 +/- 0.29 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:33.91 +42:17:09.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J051833.80+421730.2,2461153.6902,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051833.80+421730.2 20260423.1902 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 04 23.1902 2461153.6902 11.74 05:24:34.69 +41:13:46.4
167.33356 3.03127 galactic Aur Second-epoch detections are separated by 3.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF J052432.31+411341.9 | 05:24:32.31 +41:13:41.8 (Gaia DR3) | SR (local) | 2458409.57910 (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.251+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:24:34.69 +41:13:46.4: 12.12 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:24:34.69 +41:13:46.4: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.61 +/- 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
ZTF J052432.31+411341.9,2461153.6902,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052432.31+411341.9 20260423.1902 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 04 23.1902 2461153.6902 11.35 05:20:41.08 +43:25:39.7
165.10918 3.67823 galactic Aur Second-epoch detections are separated by 1.1" and 6.8 pix
The object was found in VSX24" ASASSN-V J052043.28+432538.9
Type: EA
# Max. Min./Amp. JD0 Period
12.270 V 12.650 V 2457441.82600 3.137980000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:41.08 +43:25:39.7: 12.37 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:41.08 +43:25:39.7: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 J052043.28+432538.9,2461153.6902,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052043.28+432538.9 20260423.1902 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.34 05:24:31.04 +42:18:55.1
166.42646 3.63039 galactic Aur 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 J081.1466+42.3220 | 05:24:32.93 +42:19:13.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.186+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:24:31.04 +42:18:55.1: 12.21 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:24:31.04 +42:18:55.1: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 J081.1466+42.3220,2461153.6902,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.1466+42.3220 20260423.1902 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.25 05:19:36.85 +42:36:22.3
165.67370 3.04930 galactic Aur 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 | ZTF J051934.33+423613.6 | 05:19:34.70 +42:36:03.0 (Gaia DR3) | RS (local) | 2458231.65210 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.185+/-0.029 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:36.85 +42:36:22.3: 13.88 +/- 0.17 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:36.85 +42:36:22.3: 12.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 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
ZTF J051934.33+423613.6,2461153.6902,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051934.33+423613.6 20260423.1902 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.12 05:18:30.28 +43:23:29.8
164.91240 3.33258 galactic Aur Second-epoch detections are separated by 1.7" and 6.7 pix
The object was found in VSX 2" Gaia DR3 207496123542148992
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.370 G 12.390 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:30.28 +43:23:29.8: 13.95 +/- 0.20 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:30.28 +43:23:29.8: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 207496123542148992,2461153.6902,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207496123542148992 20260423.1902 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 04 23.1902 2461153.6902 11.03 05:18:09.68 +42:30:21.8
165.60233 2.77266 galactic Aur Second-epoch detections are separated by 1.5" and 6.8 pix
The object was found in VSX18" Gaia DR3 207208674270841728
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.120 G 14.140 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:09.68 +42:30:21.8: 14.51 +/- 0.31 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:09.68 +42:30:21.8: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 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 207208674270841728,2461153.6902,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207208674270841728 20260423.1902 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.37 05:17:21.25 +43:43:46.9
164.51527 3.35634 galactic Aur Second-epoch detections are separated by 0.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.3198+43.7266 | 05:17:19.36 +43:43:36.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.275+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:21.25 +43:43:46.9: 14.31 +/- 0.25 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:21.25 +43:43:46.9: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3198+43.7266,2461153.6902,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3198+43.7266 20260423.1902 10.37CV 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 04 23.1902 2461153.6902 8.37 05:16:52.88 +42:07:31.6
165.77711 2.35990 galactic Aur Second-epoch detections are separated by 1.6" and 6.8 pix
The object was found in VSX 3" Gaia DR3 207176582275392896
Type: ACV|roAm|
# Max. Min./Amp. JD0 Period
9.350 G 9.410 G B
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:16:52.88 +42:07:31.6: 12.48 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:16:52.88 +42:07:31.6: 9.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.41 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207176582275392896,2461153.6902,8.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207176582275392896 20260423.1902 8.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 8.49 05:17:50.18 +41:52:05.9
166.08977 2.35645 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was found in VSX 4" STARE aur0 210
Type: EA
# Max. Min./Amp. JD0 Period
9.500 R Y 0.150 R 5.586590000000 B8
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:50.18 +41:52:05.9: 12.10 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:50.18 +41:52:05.9: 9.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.54 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STARE aur0 210,2461153.6902,8.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 210 20260423.1902 8.49CV 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 04 23.1902 2461153.6902 8.94 05:19:47.63 +40:57:28.0
167.04678 2.13444 galactic Aur Second-epoch detections are separated by 0.2" and 6.9 pix
The object was found in VSX21" Gaia DR3 194861772867128960
Type: ROT
# Max. Min./Amp. JD0 Period
16.750 G 16.770 G 0.758700000000 F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:47.63 +40:57:28.0: 10.29 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:47.63 +40:57:28.0: 9.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.00 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194861772867128960,2461153.6902,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194861772867128960 20260423.1902 8.94CV 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 04 23.1902 2461153.6902 9.01 05:21:11.83 +40:58:15.5
167.18712 2.35959 galactic Aur Second-epoch detections are separated by 0.3" 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 194835457606280320 | 05:21:11.97 +40:58:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+40 1258 J-Ks=0.017+/-0.032 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:11.83 +40:58:15.5: 9.48 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:11.83 +40:58:15.5: 10.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.89 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194835457606280320,2461153.6902,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194835457606280320 20260423.1902 9.01CV 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 04 23.1902 2461153.6902 9.45 05:19:37.57 +41:21:38.6
166.69794 2.33902 galactic Aur Second-epoch detections are separated by 0.0" and 6.9 pix
The object was found in VSX 1" Gaia DR3 194908437690158080
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.460 G 10.480 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:37.57 +41:21:38.6: 11.32 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:37.57 +41:21:38.6: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194908437690158080,2461153.6902,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194908437690158080 20260423.1902 9.45CV 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 04 23.1902 2461153.6902 9.56 05:17:56.22 +41:11:56.5
166.64813 1.98635 galactic Aur Second-epoch detections are separated by 0.9" and 6.9 pix
The object was found in VSX 7" STARE aur0 543
Type: DSCT
# Max. Min./Amp. JD0 Period
10.160 R Y 0.010 R 0.039040000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:56.22 +41:11:56.5: 12.56 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:56.22 +41:11:56.5: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.50 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STARE aur0 543,2461153.6902,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 543 20260423.1902 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 9.66 05:18:09.76 +40:56:38.3
166.88128 1.87426 galactic Aur Second-epoch detections are separated by 0.3" 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 194873150239029504 | 05:18:09.83 +40:56:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1949AnHar.112....1C HD 277905 J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:09.76 +40:56:38.3: 12.62 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:09.76 +40:56:38.3: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194873150239029504,2461153.6902,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194873150239029504 20260423.1902 9.66CV 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 04 23.1902 2461153.6902 9.69 05:17:58.67 +41:54:50.1
166.06762 2.40424 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195169021946272512 | 05:17:58.74 +41:54:48.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 277877 J-Ks=0.027+/-0.033 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:58.67 +41:54:50.1: 12.81 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:58.67 +41:54:50.1: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.74 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195169021946272512,2461153.6902,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195169021946272512 20260423.1902 9.69CV 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 04 23.1902 2461153.6902 9.69 05:17:04.59 +41:49:58.0
166.03713 2.22037 galactic Aur Second-epoch detections are separated by 0.6" and 6.9 pix
The object was found in VSX 2" STARE aur0 1045
Type: DSCT
# Max. Min./Amp. JD0 Period
10.570 R Y 0.020 R 0.069680000000 F0V
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:04.59 +41:49:58.0: 14.42 +/- 0.34 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:04.59 +41:49:58.0: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STARE aur0 1045,2461153.6902,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 1045 20260423.1902 9.69CV 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 04 23.1902 2461153.6902 9.77 05:19:09.52 +41:39:36.5
166.40209 2.43869 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195104253841468928 | 05:19:09.62 +41:39:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S [S28] 482 J-Ks=0.010+/-0.030 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:09.52 +41:39:36.5: 12.34 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:09.52 +41:39:36.5: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195104253841468928,2461153.6902,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195104253841468928 20260423.1902 9.77CV 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 04 23.1902 2461153.6902 9.76 05:20:34.14 +41:32:12.4
166.65423 2.58459 galactic Aur Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194914347565063040 | 05:20:34.12 +41:32:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S [S28] 489 J-Ks=0.159+/-0.039 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:34.14 +41:32:12.4: 11.34 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:34.14 +41:32:12.4: 10.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194914347565063040,2461153.6902,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194914347565063040 20260423.1902 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 9.94 05:19:17.13 +41:01:57.9
166.93032 2.09871 galactic Aur Second-epoch detections are separated by 0.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194865728535472768 | 05:19:17.25 +41:01:56.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S [S28] 484 J-Ks=0.013+/-0.033 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:17.13 +41:01:57.9: 11.82 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:17.13 +41:01:57.9: 10.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.02 +/- 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 194865728535472768,2461153.6902,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194865728535472768 20260423.1902 9.94CV 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 04 23.1902 2461153.6902 10.01 05:17:43.68 +41:05:44.2
166.71001 1.89460 galactic Aur Second-epoch detections are separated by 0.3" and 6.9 pix
The object was found in VSX 5" STARE aur0 1639
Type: BCEP
# Max. Min./Amp. JD0 Period
10.940 R Y 0.040 R 0.486860000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:43.68 +41:05:44.2: 13.57 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:43.68 +41:05:44.2: 11.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 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
STARE aur0 1639,2461153.6902,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 1639 20260423.1902 10.01CV 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 04 23.1902 2461153.6902 10.05 05:20:36.24 +41:26:10.9
166.74057 2.53276 galactic Aur Second-epoch detections are separated by 0.2" and 6.8 pix
The object was found in VSX 2" STARE aur0 830
Type: I
# Max. Min./Amp. JD0 Period
10.800 R Y 0.300 R 16.666700000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:36.24 +41:26:10.9: 11.42 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:36.24 +41:26:10.9: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 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
STARE aur0 830,2461153.6902,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 830 20260423.1902 10.05CV 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 04 23.1902 2461153.6902 10.02 05:19:59.12 +40:55:10.5
167.09883 2.14228 galactic Aur 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 J080.0126+40.9176 | 05:19:59.24 +40:55:08.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 1949AnHar.112....1C HD 277910 J-Ks=0.223+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:59.12 +40:55:10.5: 11.21 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:59.12 +40:55:10.5: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.0126+40.9176,2461153.6902,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.0126+40.9176 20260423.1902 10.02CV 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 04 23.1902 2461153.6902 10.02 05:17:27.03 +42:04:46.0
165.87571 2.41954 galactic Aur 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 | Gaia DR3 195163245211271168 | 05:17:27.14 +42:04:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S [S28] 472
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:27.03 +42:04:46.0: 13.74 +/- 0.16 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:27.03 +42:04:46.0: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.07 +/- 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 195163245211271168,2461153.6902,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195163245211271168 20260423.1902 10.02CV 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 04 23.1902 2461153.6902 10.04 05:21:26.78 +41:09:41.1
167.05699 2.50646 galactic Aur Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.3487+41.1656 | 05:21:26.78 +41:09:43.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 1949AnHar.112....1C HD 278051 J-Ks=0.178+/-0.024 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:26.78 +41:09:41.1: 10.94 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:26.78 +41:09:41.1: 11.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.3487+41.1656,2461153.6902,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.3487+41.1656 20260423.1902 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.07 05:21:19.27 +40:58:22.2
167.19891 2.37990 galactic Aur Second-epoch detections are separated by 0.7" and 7.0 pix
The object was found in VSX 2" Gaia DR3 194835522027653632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.070 G 11.090 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:19.27 +40:58:22.2: 10.62 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:19.27 +40:58:22.2: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.02 +/- 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 194835522027653632,2461153.6902,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194835522027653632 20260423.1902 10.07CV 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 04 23.1902 2461153.6902 10.14 05:19:32.68 +41:34:44.4
166.51001 2.45138 galactic Aur 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 | Gaia DR3 195100027592029568 | 05:19:32.82 +41:34:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.101+/-0.029 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:32.68 +41:34:44.4: 12.36 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:32.68 +41:34:44.4: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 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 195100027592029568,2461153.6902,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195100027592029568 20260423.1902 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.14 05:19:44.90 +41:25:28.8
166.65855 2.39439 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.9448+41.4225 | 05:19:44.98 +41:25:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:44.90 +41:25:28.8: 11.97 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:44.90 +41:25:28.8: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.9448+41.4225,2461153.6902,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.9448+41.4225 20260423.1902 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.21 05:19:31.24 +41:15:46.4
166.76689 2.26680 galactic Aur Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194881598437726336 | 05:19:31.31 +41:15:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.356+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:31.24 +41:15:46.4: 12.28 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:31.24 +41:15:46.4: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 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 194881598437726336,2461153.6902,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194881598437726336 20260423.1902 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.21 05:20:09.95 +41:28:55.1
166.65620 2.49133 galactic Aur Second-epoch detections are separated by 0.2" and 6.8 pix
The object was found in VSX15" ZTF J052009.88+412910.1
Type: EW
# Max. Min./Amp. JD0 Period
17.657 r Y 0.465 r 2458522.70200 0.306726400000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:09.95 +41:28:55.1: 12.15 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:09.95 +41:28:55.1: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 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
ZTF J052009.88+412910.1,2461153.6902,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052009.88+412910.1 20260423.1902 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.19 05:19:26.45 +41:33:40.0
166.51357 2.42522 galactic Aur Second-epoch detections are separated by 0.1" 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 | Gaia DR3 195099890153078912 | 05:19:26.56 +41:33:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 277889 J-Ks=0.058+/-0.030 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:26.45 +41:33:40.0: 12.59 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:26.45 +41:33:40.0: 11.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 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 195099890153078912,2461153.6902,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195099890153078912 20260423.1902 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 04 23.1902 2461153.6902 10.20 05:17:39.16 +41:50:01.0
166.09843 2.30851 galactic Aur Second-epoch detections are separated by 0.5" and 6.9 pix
The object was found in VSX 2" Gaia DR3 195144557812620160
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.270 G 11.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:39.16 +41:50:01.0: 12.60 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:39.16 +41:50:01.0: 11.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 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 195144557812620160,2461153.6902,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195144557812620160 20260423.1902 10.20CV 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 04 23.1902 2461153.6902 10.24 05:18:00.23 +41:05:42.0
166.74047 1.93672 galactic Aur Second-epoch detections are separated by 0.2" and 6.9 pix
The object was found in VSX 3" Gaia DR3 195062815995460096
Type: E
# Max. Min./Amp. JD0 Period
11.320 G 11.420 G 2.194350000000 B
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:00.23 +41:05:42.0: 12.47 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:00.23 +41:05:42.0: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 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 195062815995460096,2461153.6902,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195062815995460096 20260423.1902 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.35 05:19:51.14 +40:54:04.5
167.09951 2.11118 galactic Aur Second-epoch detections are separated by 0.2" 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 | Gaia DR3 194861085672994816 | 05:19:51.11 +40:54:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.238+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:51.14 +40:54:04.5: 11.55 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:51.14 +40:54:04.5: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194861085672994816,2461153.6902,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194861085672994816 20260423.1902 10.35CV 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 04 23.1902 2461153.6902 10.34 05:17:57.77 +41:10:44.5
166.66729 1.97880 galactic Aur 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 | Gaia DR3 195065457395369216 | 05:17:57.88 +41:10:43.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.118+/-0.028 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:57.77 +41:10:44.5: 13.54 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:57.77 +41:10:44.5: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 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 195065457395369216,2461153.6902,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195065457395369216 20260423.1902 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.37 05:18:13.00 +41:37:19.8
166.33208 2.27279 galactic Aur Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.5652+41.6227 | 05:18:13.09 +41:37:20.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.030 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:13.00 +41:37:19.8: 13.74 +/- 0.15 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:13.00 +41:37:19.8: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5652+41.6227,2461153.6902,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5652+41.6227 20260423.1902 10.37CV 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 04 23.1902 2461153.6902 10.32 05:21:47.64 +41:19:19.6
166.96168 2.65147 galactic Aur Second-epoch detections are separated by 0.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194850331075823104 | 05:21:47.70 +41:19:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.205+/-0.023 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:47.64 +41:19:19.6: 11.08 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:47.64 +41:19:19.6: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 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 194850331075823104,2461153.6902,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194850331075823104 20260423.1902 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.36 05:19:09.37 +41:40:20.0
166.39191 2.44524 galactic Aur Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195104253841468928 | 05:19:09.62 +41:39:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S [S28] 482 J-Ks=0.074+/-0.030 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:09.37 +41:40:20.0: 12.80 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:09.37 +41:40:20.0: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 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 195104253841468928,2461153.6902,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195104253841468928 20260423.1902 10.36CV 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 04 23.1902 2461153.6902 10.38 05:18:09.11 +42:18:27.1
165.76394 2.65709 galactic Aur 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 | Gaia DR3 195193344342077824 | 05:18:09.20 +42:18:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.073+/-0.033 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:09.11 +42:18:27.1: 13.83 +/- 0.16 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:09.11 +42:18:27.1: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 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 195193344342077824,2461153.6902,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195193344342077824 20260423.1902 10.38CV 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 04 23.1902 2461153.6902 10.32 05:21:28.74 +41:03:43.8
167.14226 2.45516 galactic Aur Second-epoch detections are separated by 0.4" and 6.9 pix
The object was found in VSX 4" STARE aur0 2302
Type: MISC
# Max. Min./Amp. JD0 Period
11.140 R Y 0.040 R 0.541710000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:28.74 +41:03:43.8: 10.86 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:28.74 +41:03:43.8: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 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
STARE aur0 2302,2461153.6902,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 2302 20260423.1902 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.36 05:17:01.76 +41:52:11.1
166.00185 2.23457 galactic Aur Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.2526+41.8636 | 05:17:01.88 +41:52:08.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7 1949AnHar.112....1C HD 277874
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:01.76 +41:52:11.1: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:01.76 +41:52:11.1: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.2526+41.8636,2461153.6902,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.2526+41.8636 20260423.1902 10.36CV 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 04 23.1902 2461153.6902 10.38 05:21:16.64 +41:18:05.5
166.92351 2.55992 galactic Aur Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.3261+41.3030 | 05:21:16.76 +41:18:05.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1949AnHar.112....1C HD 278044 J-Ks=0.049+/-0.033 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:16.64 +41:18:05.5: 11.24 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:16.64 +41:18:05.5: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.3261+41.3030,2461153.6902,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.3261+41.3030 20260423.1902 10.38CV 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 04 23.1902 2461153.6902 10.44 05:17:38.02 +41:40:02.0
166.23245 2.20969 galactic Aur Second-epoch detections are separated by 1.0" and 6.8 pix
The object was found in VSX 2" Gaia DR3 195096243721471360
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.420 G 11.470 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:38.02 +41:40:02.0: 14.44 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:38.02 +41:40:02.0: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195096243721471360,2461153.6902,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195096243721471360 20260423.1902 10.44CV 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 04 23.1902 2461153.6902 10.42 05:21:03.45 +40:57:03.1
167.18866 2.32646 galactic Aur 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 | Gaia DR3 194838000229482368 | 05:21:03.62 +40:57:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.256+/-0.032 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:03.45 +40:57:03.1: 10.92 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:03.45 +40:57:03.1: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 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 194838000229482368,2461153.6902,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194838000229482368 20260423.1902 10.42CV 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 04 23.1902 2461153.6902 10.48 05:20:57.31 +41:19:28.7
166.87005 2.52330 galactic Aur Second-epoch detections are separated by 3.5" and 6.6 pix
The object was found in VSX 7" Gaia DR3 194899435438651904
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.020 G 12.050 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:57.31 +41:19:28.7: 11.47 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:57.31 +41:19:28.7: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194899435438651904,2461153.6902,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194899435438651904 20260423.1902 10.48CV 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 04 23.1902 2461153.6902 10.47 05:19:30.54 +41:29:14.0
166.58152 2.39339 galactic Aur Second-epoch detections are separated by 0.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.8696+41.4876 | 05:19:30.67 +41:29:15.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:30.54 +41:29:14.0: 12.82 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:30.54 +41:29:14.0: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.8696+41.4876,2461153.6902,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.8696+41.4876 20260423.1902 10.47CV 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 04 23.1902 2461153.6902 10.59 05:17:22.75 +42:24:38.3
165.59727 2.59977 galactic Aur Second-epoch detections are separated by 2.5" 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 J079.3540+42.4112 | 05:17:22.83 +42:24:36.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.085+/-0.031 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:22.75 +42:24:38.3: 13.67 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:22.75 +42:24:38.3: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3540+42.4112,2461153.6902,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3540+42.4112 20260423.1902 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.55 05:20:27.78 +41:00:57.8
167.07108 2.27138 galactic Aur Second-epoch detections are separated by 0.3" 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 194862807960593664 | 05:20:27.89 +41:00:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.445+/-0.035 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:27.78 +41:00:57.8: 11.51 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:27.78 +41:00:57.8: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 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 194862807960593664,2461153.6902,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194862807960593664 20260423.1902 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 04 23.1902 2461153.6902 10.55 05:20:09.00 +41:38:29.3
166.52341 2.57994 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.0311+41.6444 | 05:20:09.06 +41:38:29.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.032 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:09.00 +41:38:29.3: 12.52 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:09.00 +41:38:29.3: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.0311+41.6444,2461153.6902,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.0311+41.6444 20260423.1902 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 04 23.1902 2461153.6902 10.60 05:18:35.38 +41:27:42.3
166.50360 2.23770 galactic Aur Second-epoch detections are separated by 0.5" 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 J079.6541+41.4521 | 05:18:35.44 +41:27:43.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.264+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:35.38 +41:27:42.3: 13.98 +/- 0.19 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:35.38 +41:27:42.3: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.6541+41.4521,2461153.6902,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6541+41.4521 20260423.1902 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.59 05:17:08.60 +41:43:48.8
166.12810 2.17130 galactic Aur 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 J079.2863+41.7292 | 05:17:08.72 +41:43:45.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1958ApJS....4....1M LF 7 +41 532
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:08.60 +41:43:48.8: 14.28 +/- 0.26 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:08.60 +41:43:48.8: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.2863+41.7292,2461153.6902,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.2863+41.7292 20260423.1902 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.62 05:19:34.02 +41:42:04.8
166.41197 2.52479 galactic Aur Second-epoch detections are separated by 1.1" and 6.8 pix
The object was found in VSX14" Gaia DR3 195101711218785920
Type: ROT
# Max. Min./Amp. JD0 Period
15.960 G 15.990 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:34.02 +41:42:04.8: 12.84 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:34.02 +41:42:04.8: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 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 195101711218785920,2461153.6902,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195101711218785920 20260423.1902 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 04 23.1902 2461153.6902 10.59 05:18:11.73 +41:06:05.5
166.75593 1.97000 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194875207525893632 | 05:18:12.12 +41:06:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:11.73 +41:06:05.5: 13.43 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:11.73 +41:06:05.5: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 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 194875207525893632,2461153.6902,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194875207525893632 20260423.1902 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.74 05:20:37.17 +41:03:53.1
167.04788 2.32339 galactic Aur 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 | Gaia DR3 194886550537237888 | 05:20:37.31 +41:03:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.224+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:37.17 +41:03:53.1: 11.52 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:37.17 +41:03:53.1: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 194886550537237888,2461153.6902,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194886550537237888 20260423.1902 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.75 05:19:41.69 +41:41:45.5
166.43003 2.54130 galactic Aur Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 195107311856552576 | 05:19:41.74 +41:41:46.7 (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=0.286+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:41.69 +41:41:45.5: 13.40 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:41.69 +41:41:45.5: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 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
Large-amplitude variable Gaia DR2 195107311856552576,2461153.6902,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 195107311856552576 20260423.1902 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.66 05:17:44.62 +41:41:19.9
166.22660 2.23895 galactic Aur 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 J079.4334+41.6991 | 05:17:44.71 +41:41:20.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.132+/-0.028 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:44.62 +41:41:19.9: 14.13 +/- 0.23 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:44.62 +41:41:19.9: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.4334+41.6991,2461153.6902,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4334+41.6991 20260423.1902 10.66CV 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 04 23.1902 2461153.6902 10.70 05:17:14.40 +41:46:08.7
166.10677 2.20846 galactic Aur Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.3106+41.7683 | 05:17:14.55 +41:46:05.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1958ApJS....4....1M LF 7 +41 535
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:14.40 +41:46:08.7: 13.85 +/- 0.17 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:14.40 +41:46:08.7: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3106+41.7683,2461153.6902,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3106+41.7683 20260423.1902 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 04 23.1902 2461153.6902 10.79 05:18:07.11 +41:46:17.0
166.19937 2.34365 galactic Aur Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195119818800980992 | 05:18:09.01 +41:46:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.100+/-0.030 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:07.11 +41:46:17.0: 13.64 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:07.11 +41:46:17.0: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 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 195119818800980992,2461153.6902,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195119818800980992 20260423.1902 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 04 23.1902 2461153.6902 10.78 05:17:40.00 +41:57:06.9
166.00317 2.37882 galactic Aur 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 | Gaia DR3 195148985919852288 | 05:17:40.19 +41:57:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:40.00 +41:57:06.9: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:40.00 +41:57:06.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 195148985919852288,2461153.6902,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195148985919852288 20260423.1902 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.84 05:18:13.74 +41:50:13.8
166.15737 2.39833 galactic Aur 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 J079.5672+41.8312 | 05:18:13.81 +41:50:11.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:13.74 +41:50:13.8: 13.93 +/- 0.19 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:13.74 +41:50:13.8: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5672+41.8312,2461153.6902,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5672+41.8312 20260423.1902 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.79 05:17:50.58 +40:59:14.2
166.81108 1.84987 galactic Aur Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 188869606293838848 | 05:17:50.66 +40:59:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.283+/-0.028 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:50.58 +40:59:14.2: 13.94 +/- 0.18 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:50.58 +40:59:14.2: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 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 188869606293838848,2461153.6902,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 188869606293838848 20260423.1902 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 04 23.1902 2461153.6902 10.78 05:17:15.88 +42:10:20.7
165.77981 2.44503 galactic Aur Second-epoch detections are separated by 1.1" and 6.8 pix
The object was found in VSX11" ZTF J051714.95+421016.6
Type: SR
# Max. Min./Amp. JD0 Period
13.680 r Y 0.168 r 2458346.85950 45.600186300000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:15.88 +42:10:20.7: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:15.88 +42:10:20.7: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 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
ZTF J051714.95+421016.6,2461153.6902,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051714.95+421016.6 20260423.1902 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.76 05:17:02.25 +41:48:42.7
166.05001 2.20236 galactic Aur Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.2673+41.8169 | 05:17:02.33 +41:48:39.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 1958ApJS....4....1M LF 7 +41 528
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:02.25 +41:48:42.7: 14.51 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:02.25 +41:48:42.7: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.2673+41.8169,2461153.6902,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.2673+41.8169 20260423.1902 10.76CV 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 04 23.1902 2461153.6902 10.80 05:17:07.88 +42:00:29.7
165.89967 2.33006 galactic Aur Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195162420577552256 | 05:17:07.96 +42:00:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0: 1958ApJS....4....1M LF 7 +41 530
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:07.88 +42:00:29.7: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:07.88 +42:00:29.7: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 195162420577552256,2461153.6902,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195162420577552256 20260423.1902 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 04 23.1902 2461153.6902 10.81 05:17:43.48 +41:35:28.2
166.30445 2.17975 galactic Aur 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 J079.4329+41.5958 | 05:17:43.48 +41:35:28.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.180+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:43.48 +41:35:28.2: 13.51 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:43.48 +41:35:28.2: 11.97 +/- 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
ATO J079.4329+41.5958,2461153.6902,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4329+41.5958 20260423.1902 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 04 23.1902 2461153.6902 10.87 05:21:53.86 +41:14:46.1
167.03538 2.62444 galactic Aur Second-epoch detections are separated by 0.2" 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 | Gaia DR3 194847651016219264 | 05:21:53.91 +41:14:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.362+/-0.024 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:53.86 +41:14:46.1: 11.73 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:53.86 +41:14:46.1: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 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 194847651016219264,2461153.6902,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194847651016219264 20260423.1902 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.86 05:20:59.01 +40:58:25.8
167.16180 2.32805 galactic Aur Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194838275104845696 | 05:20:59.16 +40:58:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.195+/-0.032 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:59.01 +40:58:25.8: 11.51 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:59.01 +40:58:25.8: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 194838275104845696,2461153.6902,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194838275104845696 20260423.1902 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.87 05:17:29.03 +41:47:23.6
166.11602 2.25759 galactic Aur Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.3715+41.7891 | 05:17:29.17 +41:47:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1958ApJS....4....1M LF 7 +41 537
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:29.03 +41:47:23.6: 14.04 +/- 0.20 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:29.03 +41:47:23.6: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3715+41.7891,2461153.6902,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3715+41.7891 20260423.1902 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.91 05:19:01.33 +41:46:25.8
166.29422 2.48298 galactic Aur Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 195117688495731328 | 05:19:01.41 +41:46:26.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A7V (LAMOST DR5) J-Ks=0.141+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:01.33 +41:46:25.8: 13.70 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:01.33 +41:46:25.8: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 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
Large-amplitude variable Gaia DR2 195117688495731328,2461153.6902,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 195117688495731328 20260423.1902 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.86 05:17:15.30 +42:00:41.2
165.91034 2.35066 galactic Aur 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 | ATO J079.3111+42.0077 | 05:17:15.38 +42:00:39.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0: 1958ApJS....4....1M LF 7 +41 533 J-Ks=0.225+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:15.30 +42:00:41.2: 14.54 +/- 0.32 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:15.30 +42:00:41.2: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3111+42.0077,2461153.6902,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3111+42.0077 20260423.1902 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.91 05:19:34.56 +41:44:04.0
166.38575 2.54511 galactic Aur Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195110576031263232 | 05:19:34.62 +41:44:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.249+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:34.56 +41:44:04.0: 13.32 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:34.56 +41:44:04.0: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 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 195110576031263232,2461153.6902,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195110576031263232 20260423.1902 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.93 05:17:03.28 +41:28:02.5
166.33321 2.00589 galactic Aur Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.2641+41.4677 | 05:17:03.39 +41:28:04.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1958ApJS....4....1M LF 7 +41 531 J-Ks=0.046+/-0.034 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:03.28 +41:28:02.5: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:03.28 +41:28:02.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.2641+41.4677,2461153.6902,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.2641+41.4677 20260423.1902 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.93 05:19:22.67 +41:06:10.6
166.88272 2.15319 galactic Aur Second-epoch detections are separated by 0.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194878093743483648 | 05:19:22.76 +41:06:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.191+/- (unrealisitic color!)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:22.67 +41:06:10.6: 12.93 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:22.67 +41:06:10.6: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 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 194878093743483648,2461153.6902,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194878093743483648 20260423.1902 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 10.94 05:17:41.78 +41:24:12.1
166.45496 2.06716 galactic Aur Second-epoch detections are separated by 0.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.4242+41.4038 | 05:17:41.82 +41:24:13.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.189+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:41.78 +41:24:12.1: 12.41 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:41.78 +41:24:12.1: 12.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.4242+41.4038,2461153.6902,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4242+41.4038 20260423.1902 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 04 23.1902 2461153.6902 10.99 05:19:09.42 +41:18:59.1
166.68382 2.24146 galactic Aur Second-epoch detections are separated by 0.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.7933+41.3189 | 05:19:09.50 +41:18:58.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.254+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:09.42 +41:18:59.1: 13.44 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:09.42 +41:18:59.1: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.7933+41.3189,2461153.6902,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.7933+41.3189 20260423.1902 10.99CV 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 04 23.1902 2461153.6902 11.02 05:18:03.55 +42:06:18.5
165.91979 2.52664 galactic Aur Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.5108+42.1102 | 05:18:03.61 +42:06:16.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:03.55 +42:06:18.5: 14.60 +/- 0.34 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:03.55 +42:06:18.5: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5108+42.1102,2461153.6902,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5108+42.1102 20260423.1902 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.03 05:17:18.76 +42:27:03.9
165.55711 2.61308 galactic Aur Second-epoch detections are separated by 2.5" 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 207218634295160192 | 05:17:18.84 +42:27:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:18.76 +42:27:03.9: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:18.76 +42:27:03.9: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 207218634295160192,2461153.6902,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207218634295160192 20260423.1902 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.04 05:19:40.99 +41:28:15.9
166.61345 2.41091 galactic Aur Second-epoch detections are separated by 0.5" and 6.8 pix
The object was found in VSX 8" Gaia DR3 194910121313400832
Type: E
# Max. Min./Amp. JD0 Period
18.860 G 19.300 G 0.330391000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:40.99 +41:28:15.9: 12.86 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:40.99 +41:28:15.9: 12.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194910121313400832,2461153.6902,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194910121313400832 20260423.1902 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.04 05:17:45.72 +41:41:57.8
166.21996 2.24781 galactic Aur 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 J079.4334+41.6991 | 05:17:44.71 +41:41:20.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=-0.002+/-0.035 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:45.72 +41:41:57.8: 12.70 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:45.72 +41:41:57.8: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.4334+41.6991,2461153.6902,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4334+41.6991 20260423.1902 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.14 05:18:24.57 +41:48:04.5
166.20614 2.40520 galactic Aur Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.6026+41.8014 | 05:18:24.64 +41:48:05.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.246+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:24.57 +41:48:04.5: 14.45 +/- 0.28 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:24.57 +41:48:04.5: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.6026+41.8014,2461153.6902,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6026+41.8014 20260423.1902 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.13 05:17:41.79 +41:03:14.7
166.74053 1.86580 galactic Aur Second-epoch detections are separated by 0.7" and 6.9 pix
The object was found in VSX 2" Gaia DR3 195062433738393728
Type: VAR
# Max. Min./Amp. JD0 Period
12.110 G 12.130 G 0.027791600000 A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:41.79 +41:03:14.7: 13.75 +/- 0.15 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:41.79 +41:03:14.7: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 195062433738393728,2461153.6902,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195062433738393728 20260423.1902 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.13 05:18:25.87 +42:08:49.6
165.92511 2.60721 galactic Aur Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.6174+42.1600 | 05:18:25.69 +42:09:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.166+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:25.87 +42:08:49.6: 14.20 +/- 0.30 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:25.87 +42:08:49.6: 12.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 J079.6174+42.1600,2461153.6902,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6174+42.1600 20260423.1902 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.12 05:18:09.63 +42:06:05.5
165.93357 2.53994 galactic Aur 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 J079.5323+42.1005 | 05:18:09.69 +42:06:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.213+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:09.63 +42:06:05.5: 14.53 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:09.63 +42:06:05.5: 12.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 J079.5323+42.1005,2461153.6902,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5323+42.1005 20260423.1902 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 04 23.1902 2461153.6902 11.19 05:18:19.13 +41:00:06.2
166.85099 1.93160 galactic Aur Second-epoch detections are separated by 1.5" and 7.1 pix
The object was found in VSX 9" Gaia DR3 194873699994828928
Type: E
# Max. Min./Amp. JD0 Period
12.870 G 13.330 G 13.159400000000 B
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:19.13 +41:00:06.2: 13.74 +/- 0.16 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:19.13 +41:00:06.2: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 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 194873699994828928,2461153.6902,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194873699994828928 20260423.1902 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 04 23.1902 2461153.6902 11.21 05:17:22.15 +41:40:33.6
166.19676 2.17441 galactic Aur 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 | Gaia DR3 195094972411720192 | 05:17:22.21 +41:40:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:22.15 +41:40:33.6: 14.47 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:22.15 +41:40:33.6: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 195094972411720192,2461153.6902,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195094972411720192 20260423.1902 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.23 05:20:13.91 +41:33:22.4
166.60223 2.54385 galactic Aur Second-epoch detections are separated by 0.5" 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 J080.0455+41.5524 | 05:20:13.99 +41:33:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:13.91 +41:33:22.4: 13.17 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:13.91 +41:33:22.4: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 J080.0455+41.5524,2461153.6902,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.0455+41.5524 20260423.1902 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.20 05:17:15.84 +41:12:38.4
166.56556 1.88966 galactic Aur 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 J079.3103+41.2100 | 05:17:16.06 +41:12:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:15.84 +41:12:38.4: 14.47 +/- 0.31 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:15.84 +41:12:38.4: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 J079.3103+41.2100,2461153.6902,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3103+41.2100 20260423.1902 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 04 23.1902 2461153.6902 11.21 05:18:36.21 +41:46:23.8
166.24985 2.41873 galactic Aur Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195116829503708032 | 05:18:36.32 +41:46:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.062+/-0.035 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:36.21 +41:46:23.8: 13.99 +/- 0.19 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:36.21 +41:46:23.8: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 195116829503708032,2461153.6902,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195116829503708032 20260423.1902 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.22 05:18:13.52 +41:41:03.5
166.28214 2.30986 galactic Aur Second-epoch detections are separated by 1.4" and 7.0 pix
The object was found in VSX17" ZTF J051814.78+414054.0
Type: EW
# Max. Min./Amp. JD0 Period
14.395 r Y 0.223 r 2458343.98740 0.495093200000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:13.52 +41:41:03.5: 13.34 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:13.52 +41:41:03.5: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 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
ZTF J051814.78+414054.0,2461153.6902,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051814.78+414054.0 20260423.1902 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.30 05:17:59.36 +42:12:01.2
165.83440 2.57083 galactic Aur 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 195190355044840576 | 05:17:59.43 +42:11:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.562+/-0.042 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:59.36 +42:12:01.2: 14.40 +/- 0.28 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:59.36 +42:12:01.2: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 195190355044840576,2461153.6902,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195190355044840576 20260423.1902 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.29 05:17:58.28 +41:41:03.5
166.25483 2.27107 galactic Aur 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 | Gaia DR3 195095766984178176 | 05:17:58.41 +41:41:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.075+/-0.033 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:58.28 +41:41:03.5: 13.98 +/- 0.18 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:58.28 +41:41:03.5: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 195095766984178176,2461153.6902,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195095766984178176 20260423.1902 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.35 05:18:59.13 +41:42:18.2
166.34670 2.43795 galactic Aur 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 J079.7461+41.7085 | 05:18:59.19 +41:42:18.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.639+/-0.033 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:59.13 +41:42:18.2: 14.17 +/- 0.23 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:59.13 +41:42:18.2: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 J079.7461+41.7085,2461153.6902,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.7461+41.7085 20260423.1902 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.30 05:21:56.13 +41:24:48.4
166.90143 2.72512 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was found in VSX 7" Gaia DR3 194898026689614592
Type: ROT
# Max. Min./Amp. JD0 Period
13.180 G 13.210 G G
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:56.13 +41:24:48.4: 12.20 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:56.13 +41:24:48.4: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 194898026689614592,2461153.6902,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194898026689614592 20260423.1902 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.30 05:19:56.49 +41:31:31.5
166.59650 2.48166 galactic Aur Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194912079823289984 | 05:19:56.57 +41:31:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.380+/-0.034 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:56.49 +41:31:31.5: 13.62 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:56.49 +41:31:31.5: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 194912079823289984,2461153.6902,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194912079823289984 20260423.1902 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.29 05:19:45.11 +41:19:52.9
166.73554 2.34158 galactic Aur Second-epoch detections are separated by 0.8" 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 | 05:19:45.11 +41:19:52.9 (user input) | T | P | (position from user input) J-Ks=0.269+/-0.040 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:45.11 +41:19:52.9: 13.01 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:45.11 +41:19:52.9: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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,2461153.6902,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.27 05:17:23.79 +40:56:49.1
166.79538 1.75777 galactic Aur Second-epoch detections are separated by 0.7" and 6.7 pix
The object was found in VSX 3" Gaia DR3 189056699371107328
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.260 G 12.280 G 0.083308800000 A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:23.79 +40:56:49.1: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:23.79 +40:56:49.1: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 189056699371107328,2461153.6902,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 189056699371107328 20260423.1902 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 04 23.1902 2461153.6902 11.32 05:17:57.69 +41:51:47.5
166.10738 2.37256 galactic Aur Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.4914+41.8651 | 05:17:57.67 +41:51:45.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.792+/-0.034 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:57.69 +41:51:47.5: 14.60 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:57.69 +41:51:47.5: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 J079.4914+41.8651,2461153.6902,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4914+41.8651 20260423.1902 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.38 05:17:22.79 +41:57:52.3
165.96208 2.34253 galactic Aur 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 J079.3451+41.9639 | 05:17:22.85 +41:57:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.144+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:22.79 +41:57:52.3: 14.47 +/- 0.31 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:22.79 +41:57:52.3: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 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 J079.3451+41.9639,2461153.6902,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3451+41.9639 20260423.1902 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 04 23.1902 2461153.6902 11.38 05:18:09.87 +41:34:39.5
166.36292 2.23920 galactic Aur Second-epoch detections are separated by 1.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195091162779273344 | 05:18:09.98 +41:34:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.171+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:09.87 +41:34:39.5: 14.54 +/- 0.33 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:09.87 +41:34:39.5: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 195091162779273344,2461153.6902,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195091162779273344 20260423.1902 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 04 23.1902 2461153.6902 11.39 05:19:19.10 +41:59:23.2
166.14865 2.65187 galactic Aur Second-epoch detections are separated by 4.7" 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 195128546174324736 | 05:19:19.57 +41:58:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=0.310+/-0.030 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:19.10 +41:59:23.2: 13.03 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:19.10 +41:59:23.2: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195128546174324736,2461153.6902,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195128546174324736 20260423.1902 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 04 23.1902 2461153.6902 11.39 05:17:20.63 +41:54:56.5
165.99813 2.30888 galactic Aur Second-epoch detections are separated by 2.0" and 6.6 pix
The object was found in VSX21" Gaia DR3 195149196377287680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.700 G 13.790 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:20.63 +41:54:56.5: 14.22 +/- 0.24 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:20.63 +41:54:56.5: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195149196377287680,2461153.6902,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195149196377287680 20260423.1902 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 04 23.1902 2461153.6902 11.40 05:19:30.19 +41:56:21.0
166.20988 2.65109 galactic Aur 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 J079.8705+41.9397 | 05:19:30.27 +41:56:21.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.282+/-0.028 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:30.19 +41:56:21.0: 14.27 +/- 0.24 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:30.19 +41:56:21.0: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 J079.8705+41.9397,2461153.6902,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.8705+41.9397 20260423.1902 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 04 23.1902 2461153.6902 11.38 05:17:51.67 +41:13:13.5
166.62241 1.98702 galactic Aur Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195065800992752128 | 05:17:51.73 +41:13:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.328+/-0.028 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:51.67 +41:13:13.5: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:51.67 +41:13:13.5: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 195065800992752128,2461153.6902,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195065800992752128 20260423.1902 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 04 23.1902 2461153.6902 11.38 05:17:23.36 +42:32:04.8
165.49692 2.67283 galactic Aur 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 J079.3505+42.5265 | 05:17:23.36 +42:32:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:23.36 +42:32:04.8: 14.08 +/- 0.21 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:23.36 +42:32:04.8: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 J079.3505+42.5265,2461153.6902,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3505+42.5265 20260423.1902 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 04 23.1902 2461153.6902 11.46 05:17:31.56 +42:08:57.1
165.82675 2.47120 galactic Aur Second-epoch detections are separated by 0.6" and 7.0 pix
The object was found in VSX 2" Gaia DR3 195166578105891072
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.550 G 13.590 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:31.56 +42:08:57.1: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:31.56 +42:08:57.1: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 195166578105891072,2461153.6902,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195166578105891072 20260423.1902 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 04 23.1902 2461153.6902 11.39 05:18:56.89 +41:23:06.9
166.60489 2.24882 galactic Aur Second-epoch detections are separated by 0.9" and 6.9 pix
The object was found in VSX15" Gaia DR3 195073398794823040
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.160 G 14.200 G B
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:56.89 +41:23:06.9: 13.49 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:56.89 +41:23:06.9: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 195073398794823040,2461153.6902,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195073398794823040 20260423.1902 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 04 23.1902 2461153.6902 11.48 05:17:41.86 +41:12:31.6
166.61420 1.95518 galactic Aur Second-epoch detections are separated by 1.5" 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 | ATO J079.4157+41.2092 | 05:17:41.86 +41:12:31.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.191+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:41.86 +41:12:31.6: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:41.86 +41:12:31.6: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.4157+41.2092,2461153.6902,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4157+41.2092 20260423.1902 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.46 05:22:02.87 +40:59:16.6
167.26436 2.50140 galactic Aur Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:22:02.87 +40:59:16.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.278+/-0.026 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:02.87 +40:59:16.6: 11.86 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:02.87 +40:59:16.6: 12.63 +/- 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
target,2461153.6902,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.44 05:19:23.07 +41:17:39.0
166.72657 2.26373 galactic Aur Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194884695110977280 | 05:19:23.21 +41:17:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.195+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:23.07 +41:17:39.0: 13.57 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:23.07 +41:17:39.0: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 194884695110977280,2461153.6902,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194884695110977280 20260423.1902 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 04 23.1902 2461153.6902 11.49 05:17:22.21 +41:36:53.2
166.24690 2.13923 galactic Aur Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.3454+41.6246 | 05:17:22.21 +41:36:53.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.107+/-0.034 (A)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:22.21 +41:36:53.2: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:22.21 +41:36:53.2: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 J079.3454+41.6246,2461153.6902,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3454+41.6246 20260423.1902 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.50 05:17:15.02 +41:43:32.7
166.14329 2.18502 galactic Aur Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195142285770881792 | 05:17:15.18 +41:43:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:15.02 +41:43:32.7: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:15.02 +41:43:32.7: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 195142285770881792,2461153.6902,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195142285770881792 20260423.1902 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.47 05:17:13.09 +41:44:46.8
166.12301 2.19200 galactic Aur 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 | 05:17:13.09 +41:44:46.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:13.09 +41:44:46.8: 11.89 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:13.09 +41:44:46.8: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 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,2461153.6902,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.52 05:17:22.91 +41:57:26.6
165.96813 2.33871 galactic Aur Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.3451+41.9639 | 05:17:22.85 +41:57:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:22.91 +41:57:26.6: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:22.91 +41:57:26.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 J079.3451+41.9639,2461153.6902,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3451+41.9639 20260423.1902 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.55 05:21:27.30 +41:18:34.6
166.93583 2.59197 galactic Aur 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 | 05:21:27.30 +41:18:34.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.365+/-0.025 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:27.30 +41:18:34.6: 12.41 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:27.30 +41:18:34.6: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 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,2461153.6902,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.46 05:17:16.80 +41:55:39.1
165.98160 2.30601 galactic Aur 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 J079.3085+41.9250 | 05:17:16.94 +41:55:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.031 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:16.80 +41:55:39.1: 13.71 +/- 0.15 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:16.80 +41:55:39.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 J079.3085+41.9250,2461153.6902,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3085+41.9250 20260423.1902 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 04 23.1902 2461153.6902 11.54 05:18:33.43 +41:04:56.1
166.81092 2.01467 galactic Aur Second-epoch detections are separated by 0.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:18:33.43 +41:04:56.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:33.43 +41:04:56.1: 14.38 +/- 0.28 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:33.43 +41:04:56.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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,2461153.6902,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.60 05:18:34.48 +41:19:31.6
166.61363 2.15709 galactic Aur Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.6533+41.3202 | 05:18:34.48 +41:19:31.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: B6 (LAMOST DR5) J-Ks=0.155+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:34.48 +41:19:31.6: 14.25 +/- 0.22 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:34.48 +41:19:31.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 J079.6533+41.3202,2461153.6902,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6533+41.3202 20260423.1902 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 04 23.1902 2461153.6902 11.62 05:18:42.48 +41:33:09.0
166.44198 2.30795 galactic Aur Second-epoch detections are separated by 0.2" and 6.9 pix
The object was found in VSX18" Gaia DR3 195078621474739584
Type: ROT
# Max. Min./Amp. JD0 Period
14.140 G 14.170 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:42.48 +41:33:09.0: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:42.48 +41:33:09.0: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 195078621474739584,2461153.6902,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195078621474739584 20260423.1902 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 04 23.1902 2461153.6902 11.90 05:31:45.51 +51:02:32.1
159.74707 9.43487 galactic Aur Second-epoch detections are separated by 0.9" and 6.9 pix
The object was found in VSX 3" Gaia DR3 213915523399735424
Type: ROT
# Max. Min./Amp. JD0 Period
13.100 G 13.120 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:31:45.51 +51:02:32.1: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:31:45.51 +51:02:32.1: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 213915523399735424,2461153.6902,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 213915523399735424 20260423.1902 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 04 23.1902 2461153.6902 11.61 05:22:15.07 +41:08:09.0
167.16409 2.61675 galactic Aur Second-epoch detections are separated by 0.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:22:15.07 +41:08:09.0 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.331+/-0.025 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:15.07 +41:08:09.0: 12.11 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:15.07 +41:08:09.0: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.57 05:19:36.72 +41:02:30.2
166.95824 2.15432 galactic Aur Second-epoch detections are separated by 1.0" and 7.0 pix
The object was found in VSX 1" ASASSN-V J051936.85+410229.6
Type: EA
# Max. Min./Amp. JD0 Period
12.930 g Y 0.360 g 2458831.93700 9.611000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:36.72 +41:02:30.2: 13.32 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:36.72 +41:02:30.2: 12.65 +/- 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
ASASSN-V J051936.85+410229.6,2461153.6902,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051936.85+410229.6 20260423.1902 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 04 23.1902 2461153.6902 11.60 05:17:25.80 +41:01:31.9
166.73486 1.80828 galactic Aur 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 J079.3578+41.0250 | 05:17:25.80 +41:01:31.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.290+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:25.80 +41:01:31.9: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:25.80 +41:01:31.9: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3578+41.0250,2461153.6902,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3578+41.0250 20260423.1902 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 04 23.1902 2461153.6902 11.72 05:17:43.47 +41:02:37.1
166.75211 1.86410 galactic Aur Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 195062433738393728 | 05:17:41.96 +41:03:13.2 (Gaia DR3) | VAR (local) | A (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:43.47 +41:02:37.1: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:43.47 +41:02:37.1: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195062433738393728,2461153.6902,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195062433738393728 20260423.1902 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 04 23.1902 2461153.6902 11.95 06:09:33.54 +43:09:03.8
169.92585 11.17879 galactic Aur Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.3896+43.1512 | 06:09:33.54 +43:09:03.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.303+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:09:33.54 +43:09:03.8: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:09:33.54 +43:09:03.8: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 J092.3896+43.1512,2461153.6902,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.3896+43.1512 20260423.1902 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 04 23.1902 2461153.6902 11.67 05:17:49.92 +41:19:53.8
166.52832 2.04661 galactic Aur Second-epoch detections are separated by 0.1" 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 | 05:17:49.92 +41:19:53.8 (user input) | T | P | (position from user input) J-Ks=0.260+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:49.92 +41:19:53.8: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:49.92 +41:19:53.8: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.73 05:17:36.05 +41:41:02.4
166.21519 2.21436 galactic Aur Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:36.05 +41:41:02.4 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.188+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:36.05 +41:41:02.4: 14.43 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:36.05 +41:41:02.4: 12.76 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.76 +/- 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,2461153.6902,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.72 05:17:42.33 +42:09:26.8
165.83920 2.50314 galactic Aur Second-epoch detections are separated by 0.4" and 6.9 pix
The object was found in VSX 2" Gaia DR3 195189908368242560
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.910 G 12.950 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:42.33 +42:09:26.8: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:42.33 +42:09:26.8: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 195189908368242560,2461153.6902,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195189908368242560 20260423.1902 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 04 23.1902 2461153.6902 11.69 05:17:29.48 +41:17:17.1
166.52699 1.96924 galactic Aur Second-epoch detections are separated by 0.1" 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 | 05:17:29.48 +41:17:17.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.327+/-0.029 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:29.48 +41:17:17.1: 14.53 +/- 0.33 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:29.48 +41:17:17.1: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.75 05:16:57.48 +42:27:00.6
165.52005 2.55913 galactic Aur Second-epoch detections are separated by 2.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:16:57.48 +42:27:00.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:16:57.48 +42:27:00.6: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:16:57.48 +42:27:00.6: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 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,2461153.6902,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.76 05:19:53.85 +41:09:16.5
166.89637 2.26299 galactic Aur Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.9741+41.1517 | 05:19:53.85 +41:09:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.317+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:53.85 +41:09:16.5: 13.19 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:53.85 +41:09:16.5: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J079.9741+41.1517,2461153.6902,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.9741+41.1517 20260423.1902 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 04 23.1902 2461153.6902 11.84 05:19:19.62 +40:59:12.5
166.97249 2.07880 galactic Aur 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 J079.8426+40.9844 | 05:19:19.62 +40:59:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.312+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:19.62 +40:59:12.5: 13.59 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:19.62 +40:59:12.5: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 J079.8426+40.9844,2461153.6902,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.8426+40.9844 20260423.1902 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.62 05:21:07.55 +41:01:50.2
167.13036 2.38243 galactic Aur Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.2769+41.0293 | 05:21:07.55 +41:01:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.194+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:07.55 +41:01:50.2: 12.08 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:07.55 +41:01:50.2: 12.72 +/- 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
ATO J080.2769+41.0293,2461153.6902,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.2769+41.0293 20260423.1902 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 04 23.1902 2461153.6902 11.71 05:17:46.25 +41:26:53.2
166.42643 2.10436 galactic Aur Second-epoch detections are separated by 1.5" 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 | ATO J079.4371+41.4492 | 05:17:46.25 +41:26:53.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:46.25 +41:26:53.2: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:46.25 +41:26:53.2: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 J079.4371+41.4492,2461153.6902,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4371+41.4492 20260423.1902 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 04 23.1902 2461153.6902 11.76 05:17:32.96 +42:23:23.0
165.63251 2.61338 galactic Aur 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 | 05:17:32.96 +42:23:23.0 (user input) | T | P | (position from user input) J-Ks=1.955+/- (Very red!)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:32.96 +42:23:23.0: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:32.96 +42:23:23.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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,2461153.6902,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.78 05:18:52.23 +41:48:27.7
166.25023 2.47924 galactic Aur Second-epoch detections are separated by 1.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:18:52.23 +41:48:27.7 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:52.23 +41:48:27.7: 14.64 +/- 0.34 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:52.23 +41:48:27.7: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.66 05:21:11.00 +41:07:23.0
167.06042 2.44392 galactic Aur 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 | target | 05:21:11.00 +41:07:23.0 (user input) | T | P | (position from user input) J-Ks=0.324+/-0.032 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:11.00 +41:07:23.0: 12.51 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:11.00 +41:07:23.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 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,2461153.6902,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.63 05:21:43.91 +40:55:58.4
167.27589 2.42104 galactic Aur 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 | 05:21:43.91 +40:55:58.4 (user input) | T | P | (position from user input) J-Ks=0.205+/-0.025 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:43.91 +40:55:58.4: 12.04 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:43.91 +40:55:58.4: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.54 +/- 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,2461153.6902,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.88 05:33:40.19 +48:17:45.2
162.27005 8.24190 galactic Aur 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 | 05:33:40.19 +48:17:45.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:33:40.19 +48:17:45.2: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:33:40.19 +48:17:45.2: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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,2461153.6902,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.71 05:22:26.82 +41:02:54.2
167.25716 2.59768 galactic Aur Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:22:26.82 +41:02:54.2 (user input) | T | P | (position from user input) J-Ks=0.271+/-0.026 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:26.82 +41:02:54.2: 12.21 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:26.82 +41:02:54.2: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 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,2461153.6902,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.79 05:18:13.49 +41:50:58.2
166.14683 2.40479 galactic Aur Second-epoch detections are separated by 1.2" and 7.1 pix
The object was found in VSX 3" Gaia DR3 195121291970731904
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.810 G 12.850 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:13.49 +41:50:58.2: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:13.49 +41:50:58.2: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 195121291970731904,2461153.6902,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195121291970731904 20260423.1902 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 04 23.1902 2461153.6902 11.74 05:18:22.38 +41:29:29.8
166.45580 2.22164 galactic Aur 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 J079.5864+41.4916 | 05:18:22.38 +41:29:29.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.289+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:22.38 +41:29:29.8: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:22.38 +41:29:29.8: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5864+41.4916,2461153.6902,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5864+41.4916 20260423.1902 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 04 23.1902 2461153.6902 11.75 05:19:39.30 +41:16:19.8
166.77373 2.29281 galactic Aur 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 J079.9211+41.2748 | 05:19:39.30 +41:16:19.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.249+/-0.029 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:39.30 +41:16:19.8: 13.02 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:39.30 +41:16:19.8: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.9211+41.2748,2461153.6902,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.9211+41.2748 20260423.1902 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.76 05:20:34.35 +41:18:00.6
166.84922 2.45029 galactic Aur 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 | ATO J080.1262+41.2983 | 05:20:30.30 +41:17:53.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.035 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:34.35 +41:18:00.6: 13.03 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:34.35 +41:18:00.6: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 J080.1262+41.2983,2461153.6902,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.1262+41.2983 20260423.1902 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 04 23.1902 2461153.6902 11.75 05:19:33.37 +41:30:24.1
166.57060 2.41178 galactic Aur Second-epoch detections are separated by 0.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:33.37 +41:30:24.1 (user input) | T | P | (position from user input) J-Ks=0.307+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:33.37 +41:30:24.1: 14.09 +/- 0.22 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:33.37 +41:30:24.1: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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,2461153.6902,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.72 05:17:22.06 +41:29:30.2
166.34719 2.06782 galactic Aur 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 J079.3396+41.4938 | 05:17:22.06 +41:29:30.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:22.06 +41:29:30.2: 14.35 +/- 0.26 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:22.06 +41:29:30.2: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 J079.3396+41.4938,2461153.6902,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3396+41.4938 20260423.1902 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 04 23.1902 2461153.6902 11.91 05:18:01.96 +41:23:18.1
166.50359 2.11007 galactic Aur 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 | 05:18:01.96 +41:23:18.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:01.96 +41:23:18.1: 14.48 +/- 0.34 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:01.96 +41:23:18.1: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.76 05:18:21.62 +41:34:57.8
166.37983 2.27208 galactic Aur Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.5902+41.5830 | 05:18:21.62 +41:34:57.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:21.62 +41:34:57.8: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:21.62 +41:34:57.8: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5902+41.5830,2461153.6902,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5902+41.5830 20260423.1902 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 04 23.1902 2461153.6902 11.89 05:21:46.28 +41:06:10.3
167.14002 2.52361 galactic Aur Second-epoch detections are separated by 0.8" 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 J080.4589+41.0994 | 05:21:46.28 +41:06:10.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.183+/-0.027 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:46.28 +41:06:10.3: 12.77 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:46.28 +41:06:10.3: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 J080.4589+41.0994,2461153.6902,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.4589+41.0994 20260423.1902 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 04 23.1902 2461153.6902 11.84 05:18:11.62 +41:27:00.6
166.47040 2.17033 galactic Aur Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.5329+41.4580 | 05:18:08.94 +41:26:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.036 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:11.62 +41:27:00.6: 14.66 +/- 0.35 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:11.62 +41:27:00.6: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 J079.5329+41.4580,2461153.6902,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5329+41.4580 20260423.1902 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.80 05:19:01.04 +41:43:45.8
166.33015 2.45676 galactic Aur Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:01.04 +41:43:45.8 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.035 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:01.04 +41:43:45.8: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:01.04 +41:43:45.8: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 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,2461153.6902,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 11.90 05:17:44.50 +42:11:19.3
165.81749 2.52662 galactic Aur 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 J079.4468+42.1830 | 05:17:44.50 +42:11:19.3 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.242+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:44.50 +42:11:19.3: 13.01 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:44.50 +42:11:19.3: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.4468+42.1830,2461153.6902,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4468+42.1830 20260423.1902 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 04 23.1902 2461153.6902 11.81 05:21:35.86 +41:17:58.9
166.95922 2.60839 galactic Aur Second-epoch detections are separated by 0.4" and 6.9 pix
The object was found in VSX12" Gaia DR3 194895724587195264
Type: ROT
# Max. Min./Amp. JD0 Period
15.190 G 15.220 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:35.86 +41:17:58.9: 12.57 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:35.86 +41:17:58.9: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 194895724587195264,2461153.6902,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194895724587195264 20260423.1902 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 04 23.1902 2461153.6902 11.87 05:17:43.54 +41:23:54.6
166.46211 2.06885 galactic Aur Second-epoch detections are separated by 0.6" and 6.8 pix
The object was found in VSX 2" Gaia DR3 195082637265085568
Type: ROT
# Max. Min./Amp. JD0 Period
12.910 G 12.930 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:43.54 +41:23:54.6: 13.88 +/- 0.19 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:43.54 +41:23:54.6: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 195082637265085568,2461153.6902,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195082637265085568 20260423.1902 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 04 23.1902 2461153.6902 12.21 06:11:06.00 +41:55:49.6
171.16597 10.88073 galactic Aur Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.7750+41.9301 | 06:11:06.00 +41:55:49.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:11:06.00 +41:55:49.6: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:11:06.00 +41:55:49.6: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 J092.7750+41.9301,2461153.6902,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.7750+41.9301 20260423.1902 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 04 23.1902 2461153.6902 11.99 05:18:45.14 +42:03:00.3
166.03887 2.60029 galactic Aur Second-epoch detections are separated by 4.1" 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 J079.6887+42.0477 | 05:18:45.14 +42:03:00.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:45.14 +42:03:00.3: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:45.14 +42:03:00.3: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 J079.6887+42.0477,2461153.6902,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6887+42.0477 20260423.1902 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 04 23.1902 2461153.6902 12.01 05:21:04.81 +41:33:48.6
166.68673 2.67843 galactic Aur Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:21:04.81 +41:33:48.6 (user input) | T | P | (position from user input) J-Ks=0.775+/-0.030 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:04.81 +41:33:48.6: 13.08 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:04.81 +41:33:48.6: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.81 05:21:17.63 +41:12:01.4
167.00857 2.50499 galactic Aur Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:21:17.63 +41:12:01.4 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:17.63 +41:12:01.4: 12.60 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:17.63 +41:12:01.4: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 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,2461153.6902,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.94 05:17:28.80 +41:49:34.7
166.08584 2.27801 galactic Aur 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 J079.3767+41.8495 | 05:17:30.37 +41:50:14.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:28.80 +41:49:34.7: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:28.80 +41:49:34.7: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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 J079.3767+41.8495,2461153.6902,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3767+41.8495 20260423.1902 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 04 23.1902 2461153.6902 11.92 05:17:04.64 +42:26:01.3
165.54624 2.56758 galactic Aur Second-epoch detections are separated by 1.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:04.64 +42:26:01.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:04.64 +42:26:01.3: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:04.64 +42:26:01.3: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461153.6902,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.90 05:20:28.44 +41:37:05.0
166.57723 2.61631 galactic Aur 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 J080.1272+41.6094 | 05:20:28.44 +41:37:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.270+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:28.44 +41:37:05.0: 13.42 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:28.44 +41:37:05.0: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 J080.1272+41.6094,2461153.6902,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.1272+41.6094 20260423.1902 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 04 23.1902 2461153.6902 11.79 05:20:28.88 +41:41:24.3
166.51877 2.65849 galactic Aur Second-epoch detections are separated by 2.3" and 7.1 pix
The object was found in VSX17" Gaia DR3 194920356224088448
Type: S
# Max. Min./Amp. JD0 Period
17.520 G 18.010 G
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:28.88 +41:41:24.3: 13.33 +/- 0.10 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:28.88 +41:41:24.3: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 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 194920356224088448,2461153.6902,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194920356224088448 20260423.1902 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 04 23.1902 2461153.6902 12.20 06:26:19.97 +41:59:11.2
172.37013 13.45680 galactic Aur 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 | target | 06:26:19.97 +41:59:11.2 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:26:19.97 +41:59:11.2: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:26:19.97 +41:59:11.2: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.96 05:21:01.13 +41:24:15.2
166.81134 2.57840 galactic Aur Second-epoch detections are separated by 1.7" and 6.6 pix
The object was found in VSX 2" Gaia DR3 194900328791825152
Type: E
# Max. Min./Amp. JD0 Period
13.050 G 13.210 G 0.588890000000 A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:01.13 +41:24:15.2: 13.14 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:01.13 +41:24:15.2: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 194900328791825152,2461153.6902,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194900328791825152 20260423.1902 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 04 23.1902 2461153.6902 11.90 05:17:48.68 +41:41:34.0
166.23068 2.25153 galactic Aur Second-epoch detections are separated by 1.0" and 6.9 pix
The object was found in VSX 2" Gaia DR3 195095663904973056
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.050 G 13.080 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:48.68 +41:41:34.0: 14.59 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:48.68 +41:41:34.0: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 195095663904973056,2461153.6902,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195095663904973056 20260423.1902 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 04 23.1902 2461153.6902 11.98 05:21:46.41 +41:09:51.6
167.08958 2.55881 galactic Aur Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:21:46.41 +41:09:51.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.270+/-0.025 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:46.41 +41:09:51.6: 12.71 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:46.41 +41:09:51.6: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.04 +/- 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,2461153.6902,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.02 05:18:23.67 +41:28:28.5
166.47206 2.21515 galactic Aur 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 J079.6071+41.4816 | 05:18:23.67 +41:28:28.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A2V (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:23.67 +41:28:28.5: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:23.67 +41:28:28.5: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 J079.6071+41.4816,2461153.6902,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6071+41.4816 20260423.1902 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 04 23.1902 2461153.6902 11.92 05:21:03.53 +41:02:20.3
167.11629 2.37680 galactic Aur Second-epoch detections are separated by 3.4" 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 | 05:21:03.53 +41:02:20.3 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:03.53 +41:02:20.3: 12.53 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:03.53 +41:02:20.3: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 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,2461153.6902,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.07 05:18:38.13 +42:14:06.1
165.87480 2.68868 galactic Aur Second-epoch detections are separated by 1.1" and 6.9 pix
The object was found in VSX 2" Gaia DR3 195189191112478464
Type: RS
# Max. Min./Amp. JD0 Period
13.200 G 13.410 G O
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:38.13 +42:14:06.1: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:38.13 +42:14:06.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 195189191112478464,2461153.6902,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195189191112478464 20260423.1902 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 04 23.1902 2461153.6902 11.97 05:19:43.62 +41:22:52.2
166.69198 2.36624 galactic Aur Second-epoch detections are separated by 2.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:43.62 +41:22:52.2 (user input) | T | P | (position from user input) J-Ks=0.267+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:43.62 +41:22:52.2: 14.02 +/- 0.22 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:43.62 +41:22:52.2: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.89 05:21:35.75 +41:24:39.2
166.86738 2.67122 galactic Aur Second-epoch detections are separated by 1.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:21:35.75 +41:24:39.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.426+/-0.025 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:35.75 +41:24:39.2: 12.79 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:35.75 +41:24:39.2: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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,2461153.6902,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.91 05:17:03.54 +42:00:52.5
165.88673 2.32275 galactic Aur Second-epoch detections are separated by 2.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:03.54 +42:00:52.5 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.263+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:03.54 +42:00:52.5: 13.35 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:03.54 +42:00:52.5: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 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,2461153.6902,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.87 05:17:59.26 +41:42:14.4
166.24047 2.28490 galactic Aur Second-epoch detections are separated by 2.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:59.26 +41:42:14.4 (user input) | T | P | (position from user input) J-Ks=0.185+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:59.26 +41:42:14.4: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:59.26 +41:42:14.4: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461153.6902,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.88 05:19:42.64 +41:26:17.8
166.64334 2.39638 galactic Aur 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 | ATO J079.9260+41.4302 | 05:19:42.64 +41:26:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.270+/-0.040 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:42.64 +41:26:17.8: 13.69 +/- 0.15 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:42.64 +41:26:17.8: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 J079.9260+41.4302,2461153.6902,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.9260+41.4302 20260423.1902 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 04 23.1902 2461153.6902 11.88 05:21:03.21 +41:27:00.1
166.77732 2.60980 galactic Aur 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 J080.2633+41.4526 | 05:21:03.21 +41:27:00.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.361+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:03.21 +41:27:00.1: 13.19 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:03.21 +41:27:00.1: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 J080.2633+41.4526,2461153.6902,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.2633+41.4526 20260423.1902 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 04 23.1902 2461153.6902 11.92 05:20:32.66 +41:09:01.5
166.96935 2.36059 galactic Aur Second-epoch detections are separated by 2.7" and 6.5 pix
The object was found in VSX 9" Gaia DR3 194888161148034688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.470 G 13.490 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:32.66 +41:09:01.5: 12.70 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:32.66 +41:09:01.5: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 194888161148034688,2461153.6902,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194888161148034688 20260423.1902 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 04 23.1902 2461153.6902 11.86 05:20:05.17 +41:14:24.8
166.84632 2.34104 galactic Aur 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 J080.0126+41.2429 | 05:20:03.03 +41:14:34.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.499+/-0.033 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:05.17 +41:14:24.8: 13.18 +/- 0.10 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:05.17 +41:14:24.8: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 J080.0126+41.2429,2461153.6902,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.0126+41.2429 20260423.1902 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 04 23.1902 2461153.6902 11.92 05:17:28.53 +41:13:52.7
166.57167 1.93405 galactic Aur 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 | 05:17:28.53 +41:13:52.7 (user input) | T | P | (position from user input) J-Ks=11.443+/- (unrealisitic color!)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:28.53 +41:13:52.7: 14.60 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:28.53 +41:13:52.7: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.95 05:20:29.97 +41:51:22.7
166.38396 2.75599 galactic Aur Second-epoch detections are separated by 3.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:20:29.97 +41:51:22.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.249+/-0.040 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:29.97 +41:51:22.7: 13.53 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:29.97 +41:51:22.7: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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,2461153.6902,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 11.99 05:19:37.73 +41:47:12.4
166.34841 2.58312 galactic Aur Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:37.73 +41:47:12.4 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.031 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:37.73 +41:47:12.4: 13.91 +/- 0.18 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:37.73 +41:47:12.4: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 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,2461153.6902,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.47 06:48:33.97 +49:51:14.5
166.23737 19.96013 galactic Aur Second-epoch detections are separated by 3.5" 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 | 06:48:33.97 +49:51:14.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:48:33.97 +49:51:14.5: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:48:33.97 +49:51:14.5: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.26 06:24:51.95 +43:32:25.8
170.79985 13.85587 galactic Aur Second-epoch detections are separated by 3.7" and 6.8 pix
The object was found in VSX 5" Gaia DR3 959072936002864000
Type: ROT
# Max. Min./Amp. JD0 Period
14.010 G 14.050 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:24:51.95 +43:32:25.8: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:24:51.95 +43:32:25.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 959072936002864000,2461153.6902,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 959072936002864000 20260423.1902 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 04 23.1902 2461153.6902 12.01 05:20:42.92 +40:54:42.0
167.18409 2.25102 galactic Aur Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194814566885440768 | 05:20:40.05 +40:54:19.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:42.92 +40:54:42.0: 12.72 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:42.92 +40:54:42.0: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 194814566885440768,2461153.6902,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194814566885440768 20260423.1902 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 04 23.1902 2461153.6902 12.20 05:47:15.81 +43:29:09.2
167.66138 7.77820 galactic Aur Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.8135+43.4866 | 05:47:15.81 +43:29:09.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:47:15.81 +43:29:09.2: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:47:15.81 +43:29:09.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 J086.8135+43.4866,2461153.6902,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.8135+43.4866 20260423.1902 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 04 23.1902 2461153.6902 12.10 05:17:52.95 +41:57:10.7
166.02544 2.41223 galactic Aur Second-epoch detections are separated by 2.5" and 6.5 pix
The object was found in VSX 2" Gaia DR3 195172320481146496
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.120 G 13.150 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:52.95 +41:57:10.7: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:52.95 +41:57:10.7: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 195172320481146496,2461153.6902,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195172320481146496 20260423.1902 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 04 23.1902 2461153.6902 12.33 06:16:36.27 +44:32:55.4
169.21642 12.93530 galactic Aur Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX 1" Gaia DR3 962371397869379840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.360 G 13.380 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:16:36.27 +44:32:55.4: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:16:36.27 +44:32:55.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 962371397869379840,2461153.6902,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962371397869379840 20260423.1902 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 04 23.1902 2461153.6902 11.86 05:17:18.71 +42:19:03.8
165.66606 2.53601 galactic Aur Second-epoch detections are separated by 4.2" and 6.6 pix
The object was found in VSX 2" Gaia DR3 207181766295898880
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.890 G 12.920 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:18.71 +42:19:03.8: 13.54 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:18.71 +42:19:03.8: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 207181766295898880,2461153.6902,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207181766295898880 20260423.1902 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 04 23.1902 2461153.6902 12.20 05:40:43.00 +48:20:10.6
162.85260 9.26301 galactic Aur Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:43.00 +48:20:10.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.368+/-0.026 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:40:43.00 +48:20:10.6: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:40:43.00 +48:20:10.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.05 05:17:33.46 +41:45:08.1
166.15474 2.24713 galactic Aur Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.3922+41.7434 | 05:17:33.46 +41:45:08.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.242+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:33.46 +41:45:08.1: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:33.46 +41:45:08.1: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 J079.3922+41.7434,2461153.6902,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3922+41.7434 20260423.1902 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 04 23.1902 2461153.6902 12.10 05:21:48.20 +41:07:18.4
167.12785 2.53930 galactic Aur Second-epoch detections are separated by 3.8" 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 | 05:21:48.20 +41:07:18.4 (user input) | T | P | (position from user input) J-Ks=0.242+/-0.028 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:48.20 +41:07:18.4: 12.71 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:48.20 +41:07:18.4: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 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,2461153.6902,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.04 05:19:05.62 +41:12:55.9
166.75972 2.17387 galactic Aur Second-epoch detections are separated by 3.5" and 6.3 pix
The object was found in VSX 1" ZTF J051905.70+411255.1
Type: EA
# Max. Min./Amp. JD0 Period
13.143 r Y 0.072 r 2458373.99660 1.241337300000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:05.62 +41:12:55.9: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:05.62 +41:12:55.9: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J051905.70+411255.1,2461153.6902,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051905.70+411255.1 20260423.1902 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 04 23.1902 2461153.6902 12.03 05:17:09.43 +41:50:12.7
166.04248 2.23500 galactic Aur 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 | 05:17:09.43 +41:50:12.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:09.43 +41:50:12.7: 14.54 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:09.43 +41:50:12.7: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.33 05:43:53.04 +47:06:14.7
164.20164 9.09447 galactic Aur Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.9886+47.0957 | 05:43:54.70 +47:05:35.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.326+/-0.035 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:43:53.04 +47:06:14.7: 13.15 +/- 0.10 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:43:53.04 +47:06:14.7: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 J085.9886+47.0957,2461153.6902,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.9886+47.0957 20260423.1902 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 04 23.1902 2461153.6902 12.04 05:17:38.65 +42:14:41.9
165.76104 2.54429 galactic Aur Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:38.65 +42:14:41.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.213+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:38.65 +42:14:41.9: 14.72 +/- 0.36 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:38.65 +42:14:41.9: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 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,2461153.6902,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.11 05:16:44.56 +42:12:54.0
165.68911 2.39072 galactic Aur Second-epoch detections are separated by 2.5" and 6.8 pix
The object was found in VSX 3" Gaia DR3 207179498553630464
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.130 G 13.160 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:16:44.56 +42:12:54.0: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:16:44.56 +42:12:54.0: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 207179498553630464,2461153.6902,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207179498553630464 20260423.1902 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 04 23.1902 2461153.6902 12.25 05:18:15.39 +41:28:35.9
166.45551 2.19518 galactic Aur 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 | 05:18:15.39 +41:28:35.9 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.344+/-0.035 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:15.39 +41:28:35.9: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:15.39 +41:28:35.9: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.28 05:20:46.01 +40:57:08.7
167.15611 2.28223 galactic Aur 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 J080.1902+40.9432 | 05:20:46.01 +40:57:08.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F3 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:46.01 +40:57:08.7: 12.93 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:46.01 +40:57:08.7: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 J080.1902+40.9432,2461153.6902,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.1902+40.9432 20260423.1902 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 04 23.1902 2461153.6902 12.16 05:22:00.78 +41:12:01.9
167.08530 2.61645 galactic Aur 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 J080.5047+41.1928 | 05:22:00.78 +41:12:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.265+/-0.027 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:00.78 +41:12:01.9: 12.72 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:00.78 +41:12:01.9: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 J080.5047+41.1928,2461153.6902,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.5047+41.1928 20260423.1902 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 04 23.1902 2461153.6902 12.06 05:19:31.37 +41:08:13.6
166.87034 2.19514 galactic Aur Second-epoch detections are separated by 1.9" and 6.7 pix
The object was found in VSX 1" Gaia DR3 194879708651186560
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.010 G 13.050 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:31.37 +41:08:13.6: 14.23 +/- 0.23 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:31.37 +41:08:13.6: 13.16 +/- 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
Gaia DR3 194879708651186560,2461153.6902,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194879708651186560 20260423.1902 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 04 23.1902 2461153.6902 12.43 05:40:17.56 +46:01:05.4
164.82558 8.00838 galactic Aur Second-epoch detections are separated by 3.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 209484933918381952 | 05:40:19.96 +46:00:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:40:17.56 +46:01:05.4: 12.90 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:40:17.56 +46:01:05.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 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 209484933918381952,2461153.6902,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209484933918381952 20260423.1902 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 04 23.1902 2461153.6902 12.23 05:22:12.40 +41:06:52.8
167.17681 2.59786 galactic Aur Second-epoch detections are separated by 2.9" 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 J080.5557+41.1177 | 05:22:12.40 +41:06:52.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:12.40 +41:06:52.8: 12.79 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:12.40 +41:06:52.8: 13.37 +/- 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
ATO J080.5557+41.1177,2461153.6902,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.5557+41.1177 20260423.1902 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 04 23.1902 2461153.6902 12.07 05:20:04.97 +41:39:14.0
166.50604 2.57672 galactic Aur Second-epoch detections are separated by 1.7" and 7.1 pix
The object was found in VSX 1" Gaia DR3 194918638236940032
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.100 G 13.140 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:04.97 +41:39:14.0: 14.18 +/- 0.21 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:04.97 +41:39:14.0: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 194918638236940032,2461153.6902,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194918638236940032 20260423.1902 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 04 23.1902 2461153.6902 12.29 05:22:56.32 +40:57:00.2
167.39085 2.61863 galactic Aur 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 | 05:22:56.32 +40:57:00.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:56.32 +40:57:00.2: 12.51 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:56.32 +40:57:00.2: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461153.6902,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.36 05:28:01.16 +48:14:58.9
161.79944 7.42412 galactic Aur Second-epoch detections are separated by 2.7" and 6.8 pix
The object was found in VSX 3" Gaia DR3 212655861031529216
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.330 G 13.360 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:28:01.16 +48:14:58.9: 13.32 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:28:01.16 +48:14:58.9: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 212655861031529216,2461153.6902,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212655861031529216 20260423.1902 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 04 23.1902 2461153.6902 12.24 05:17:44.79 +41:17:54.0
166.54627 2.01431 galactic Aur Second-epoch detections are separated by 2.3" 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 | ATO J079.4287+41.2889 | 05:17:44.79 +41:17:54.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.439+/-0.030 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:44.79 +41:17:54.0: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:44.79 +41:17:54.0: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 J079.4287+41.2889,2461153.6902,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4287+41.2889 20260423.1902 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 04 23.1902 2461153.6902 12.40 05:20:41.60 +49:23:44.5
160.16481 7.05333 galactic Aur Second-epoch detections are separated by 4.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:20:41.60 +49:23:44.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:41.60 +49:23:44.5: 14.55 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:41.60 +49:23:44.5: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.27 05:21:02.28 +40:59:50.8
167.14823 2.34994 galactic Aur 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 J080.2575+40.9928 | 05:21:02.28 +40:59:50.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:02.28 +40:59:50.8: 12.83 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:02.28 +40:59:50.8: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.2575+40.9928,2461153.6902,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.2575+40.9928 20260423.1902 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 04 23.1902 2461153.6902 12.59 05:47:22.10 +46:02:51.4
165.43134 9.08081 galactic Aur Second-epoch detections are separated by 3.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.8430+46.0503 | 05:47:22.10 +46:02:51.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:47:22.10 +46:02:51.4: 13.72 +/- 0.13 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:47:22.10 +46:02:51.4: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 J086.8430+46.0503,2461153.6902,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.8430+46.0503 20260423.1902 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 12.09 05:20:00.07 +41:39:11.7
166.49785 2.56383 galactic Aur Second-epoch detections are separated by 1.8" and 6.8 pix
The object was found in VSX14" Gaia DR3 195106281064400000
Type: S
# Max. Min./Amp. JD0 Period
17.890 G 19.160 G
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:00.07 +41:39:11.7: 13.21 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:00.07 +41:39:11.7: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 195106281064400000,2461153.6902,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195106281064400000 20260423.1902 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 04 23.1902 2461153.6902 12.28 05:20:56.82 +41:41:27.6
166.56757 2.73048 galactic Aur Second-epoch detections are separated by 3.3" and 7.4 pix
The object was found in VSX14" Gaia DR3 194916958905115264
Type: RS
# Max. Min./Amp. JD0 Period
15.930 G 16.080 G 2.909900000000 K
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:56.82 +41:41:27.6: 13.58 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:56.82 +41:41:27.6: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 194916958905115264,2461153.6902,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194916958905115264 20260423.1902 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 04 23.1902 2461153.6902 12.27 05:19:18.46 +41:43:23.0
166.36641 2.49753 galactic Aur Second-epoch detections are separated by 0.9" and 7.1 pix
The object was found in VSX10" Gaia DR3 195104872314721408
Type: ROT
# Max. Min./Amp. JD0 Period
15.180 G 15.210 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:18.46 +41:43:23.0: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:18.46 +41:43:23.0: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 195104872314721408,2461153.6902,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195104872314721408 20260423.1902 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 04 23.1902 2461153.6902 12.29 05:18:48.90 +41:33:08.5
166.45359 2.32426 galactic Aur Second-epoch detections are separated by 2.4" and 6.6 pix
The object was found in VSX 2" Gaia DR3 195102054816294272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.330 G 13.350 G F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:48.90 +41:33:08.5: 14.49 +/- 0.30 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:48.90 +41:33:08.5: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 195102054816294272,2461153.6902,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195102054816294272 20260423.1902 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 04 23.1902 2461153.6902 12.22 05:18:33.51 +40:55:58.4
166.93337 1.92904 galactic Aur Second-epoch detections are separated by 5.2" and 7.6 pix
The object was found in VSX18" Gaia DR3 194869572528984448
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.770 G 13.800 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:33.51 +40:55:58.4: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:33.51 +40:55:58.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 194869572528984448,2461153.6902,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194869572528984448 20260423.1902 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 04 23.1902 2461153.6902 12.29 05:18:19.07 +42:20:17.5
165.75647 2.69982 galactic Aur Second-epoch detections are separated by 3.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.5892+42.3348 | 05:18:19.07 +42:20:17.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:19.07 +42:20:17.5: 13.99 +/- 0.18 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:19.07 +42:20:17.5: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5892+42.3348,2461153.6902,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5892+42.3348 20260423.1902 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 04 23.1902 2461153.6902 12.23 05:21:14.48 +41:05:09.5
167.09718 2.43182 galactic Aur Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.2971+41.0906 | 05:21:14.48 +41:05:09.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:14.48 +41:05:09.5: 12.78 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:14.48 +41:05:09.5: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 J080.2971+41.0906,2461153.6902,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.2971+41.0906 20260423.1902 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 04 23.1902 2461153.6902 12.31 05:18:47.20 +41:36:34.4
166.40367 2.35274 galactic Aur Second-epoch detections are separated by 1.3" and 6.8 pix
The object was found in VSX 3" Gaia DR3 195103016888944256
Type: ROT
# Max. Min./Amp. JD0 Period
13.290 G 13.320 G G
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:47.20 +41:36:34.4: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:47.20 +41:36:34.4: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 195103016888944256,2461153.6902,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195103016888944256 20260423.1902 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 04 23.1902 2461153.6902 12.34 05:17:16.13 +41:16:54.2
166.50804 1.93144 galactic Aur Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:16.13 +41:16:54.2 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.291+/-0.036 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:16.13 +41:16:54.2: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:16.13 +41:16:54.2: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.35 05:17:45.94 +42:13:18.5
165.79296 2.54933 galactic Aur Second-epoch detections are separated by 4.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:45.94 +42:13:18.5 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.031 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:45.94 +42:13:18.5: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:45.94 +42:13:18.5: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 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,2461153.6902,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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 04 23.1902 2461153.6902 12.29 05:18:20.57 +41:53:19.0
166.12744 2.44525 galactic Aur Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.5686+41.8864 | 05:18:20.57 +41:53:19.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A0III (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:20.57 +41:53:19.0: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:20.57 +41:53:19.0: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 J079.5686+41.8864,2461153.6902,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5686+41.8864 20260423.1902 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 04 23.1902 2461153.6902 12.55 05:20:34.96 +40:57:01.5
167.13793 2.25251 galactic Aur Second-epoch detections are separated by 1.8" and 7.0 pix
The object was found in VSX 4" Gaia DR3 194815391519143680
Type: ROT
# Max. Min./Amp. JD0 Period
13.630 G 13.660 G 2.723680000000 F
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:34.96 +40:57:01.5: 13.03 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:34.96 +40:57:01.5: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 194815391519143680,2461153.6902,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194815391519143680 20260423.1902 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 12.41 05:18:13.25 +41:29:51.2
166.43454 2.20175 galactic Aur Second-epoch detections are separated by 2.7" 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 J079.5555+41.4951 | 05:18:13.25 +41:29:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:13.25 +41:29:51.2: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:13.25 +41:29:51.2: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 J079.5555+41.4951,2461153.6902,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5555+41.4951 20260423.1902 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 04 23.1902 2461153.6902 12.86 06:12:44.60 +47:30:42.7
166.17207 13.60569 galactic Aur 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 | Gaia DR3 968792687512124800 | 06:12:42.84 +47:30:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:12:44.60 +47:30:42.7: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:12:44.60 +47:30:42.7: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 968792687512124800,2461153.6902,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968792687512124800 20260423.1902 12.86CV 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 04 23.1902 2461153.6902 12.97 06:13:33.56 +48:03:18.0
165.72717 13.96219 galactic Aur 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 | Gaia DR3 968835396666764416 | 06:13:35.06 +48:02:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5) J-Ks=0.403+/-0.031 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:13:33.56 +48:03:18.0: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:13:33.56 +48:03:18.0: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 968835396666764416,2461153.6902,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968835396666764416 20260423.1902 12.97CV 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 04 23.1902 2461153.6902 12.93 06:01:16.84 +47:35:44.3
165.21228 11.91132 galactic Aur Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.3023+47.5982 | 06:01:16.84 +47:35:44.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:01:16.84 +47:35:44.3: 14.91 +/- 0.36 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:01:16.84 +47:35:44.3: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 J090.3023+47.5982,2461153.6902,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.3023+47.5982 20260423.1902 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195273578630514560,2461153.6902,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195273578630514560 20260423.1902 10.45CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STARE aur0 5793,2461153.6902,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
STARE aur0 5793 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.6174+42.1600,2461153.6902,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6174+42.1600 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.3149+41.0905,2461153.6902,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.3149+41.0905 20260423.1902 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 04 23.1902 2461153.6902 12.23 05:22:21.30 +41:29:28.5
166.88178 2.83397 galactic Aur Second-epoch detections are separated by 1.8" and 7.1 pix
The object was found in VSX 1" Gaia DR3 194945546208281472
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.220 G 13.260 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:21.30 +41:29:28.5: 12.84 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:21.30 +41:29:28.5: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194945546208281472,2461153.6902,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194945546208281472 20260423.1902 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 04 23.1902 2461153.6902 10.29 05:17:39.42 +41:49:36.5
166.10446 2.30524 galactic Aur Second-epoch detections are separated by 1.0" and 6.8 pix
The object was found in VSX23" Gaia DR3 195144557812620160
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.270 G 11.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:39.42 +41:49:36.5: 12.33 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:39.42 +41:49:36.5: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 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 195144557812620160,2461153.6902,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195144557812620160 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.2136+41.7512,2461153.6902,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.2136+41.7512 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195212310918384128,2461153.6902,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195212310918384128 20260423.1902 11.11CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195144557812620160,2461153.6902,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195144557812620160 20260423.1902 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5329+41.4580,2461153.6902,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.5329+41.4580 20260423.1902 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VY Aur,2461153.6902,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VY Aur 20260423.1902 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.3306+44.0131,2461153.6902,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.3306+44.0131 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.4894+41.3942,2461153.6902,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.4894+41.3942 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.0336+41.5679,2461153.6902,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.0336+41.5679 20260423.1902 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 04 23.1902 2461153.6902 11.90 05:17:46.24 +41:44:25.9
166.18725 2.27284 galactic Aur 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 | target | 05:17:46.24 +41:44:25.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.194+/-0.039 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:46.24 +41:44:25.9: 14.12 +/- 0.20 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:46.24 +41:44:25.9: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 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,2461153.6902,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194839988794566528,2461153.6902,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194839988794566528 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195112259658390656,2461153.6902,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195112259658390656 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.2867+41.9511,2461153.6902,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.2867+41.9511 20260423.1902 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.1902 2461153.6902 12.12 05:18:06.86 +41:54:42.3
166.08402 2.42377 galactic Aur Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:18:06.86 +41:54:42.3 (user input) | T | P | (position from user input) J-Ks=0.183+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:18:06.86 +41:54:42.3: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:18:06.86 +41:54:42.3: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.7880+41.3772,2461153.6902,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.7880+41.3772 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194182244620135168,2461153.6902,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194182244620135168 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.6902,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260423.1902 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195174828741921280,2461153.6902,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195174828741921280 20260423.1902 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.6267+42.9223,2461153.6902,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.6267+42.9223 20260423.1902 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.2557+43.1607,2461153.6902,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.2557+43.1607 20260423.1902 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461153.69058979 23.04.2026 04:34:16.958 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 6 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): 22904
Objects passed selection criteria: 22800
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 16422.2
Average stars matched: 15956.2 (97.1624 %)
Memory usage VmPeak: 126884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 22 23:36:53 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: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461153.69058979 23.04.2026 04:34:16.958 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 707
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 66 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): 156651
Objects passed selection criteria: 156316
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 121037
Average stars matched: 116907 (96.5882 %)
Memory usage VmPeak: 1982080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 22 23:42:50 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.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: 2461153.68980222
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 935.1'x631.3' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 05:59:47.823 +46:00:35.63 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:47.028 +45:55:19.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 05:59:47.028 +45:55:19.19
Angular distance between the image centers 0.0879 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:47.731 +45:56:00.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 05:59:47.731 +45:56:00.01
Angular distance between the image centers 0.0766 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:59:47.028 +45:55:19.19
Second-epoch second image center 05:59:47.731 +45:56:00.01
Angular distance between the image centers 0.01152 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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.dR9B7u0COY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.meg9md0Mbe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits &> /tmp/tmp.Tk9NAPVYpb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits &> /tmp/tmp.YEbLRbbcuT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 24266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9190 to 102.4864 deg, Dec +39.9773 to +51.3461 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 77.9190 to 102.4864 deg, Dec 39.9773 to 51.3461 deg
Loaded 11816 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): 86 out of 101 total matches.
Matched with Tycho-2 101 out of 24266 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 23.040760
a=0.000000 b=1.000000 c=23.040760
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9190 to 102.4864 deg, Dec +39.9773 to +51.3461 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 77.9190 to 102.4864 deg, Dec 39.9773 to 51.3461 deg
Loaded 11816 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): 86 out of 101 total matches.
Matched with Tycho-2 101 out of 24266 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (aperture=6.0)
Read 24282 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9146 to 102.6261 deg, Dec +39.9574 to +51.3456 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 77.9146 to 102.6261 deg, Dec 39.9574 to 51.3456 deg
Loaded 11915 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): 8035 out of 8916 total matches.
Matched with Tycho-2 8916 out of 24282 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 91 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.3 pix fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
2.3 pix fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
2.1 pix wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.2 mag. fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
14.1 mag. fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (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.dR9B7u0COY (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2260, passed=24266
Got 24266 stars (including 21982 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 24266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 417 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 363 matched stars entering correct_measured_positions(), 321 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 354 matched stars entering correct_measured_positions(), 9707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.36"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 406 matched stars entering correct_measured_positions(), 9733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.27"
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 10903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.47"
Excluding outliers - 405 stars left (next iteration limit 389)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.meg9md0Mbe (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2222, passed=24282
Got 24282 stars (including 22031 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 24282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.Tk9NAPVYpb (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=584, passed=8967
Got 8967 stars (including 8369 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat
util/solve_plate_with_UCAC5 got 8967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 8763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 8763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 8761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.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.YEbLRbbcuT (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=483, passed=8583
Got 8583 stars (including 8084 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 8583 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 8370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 8370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 8370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.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_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out04959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16670.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 2s
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Considering the candidate 31503_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31503_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:02.53 +42:11:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31504_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31504_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:14.60 +41:05:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31505_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31505_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:55.47 +41:05:46.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31513_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31513_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:40.61 +41:13:13.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31514_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31514_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:55.34 +40:59:01.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31515_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31515_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:51.20 +41:14:30.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31516_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31516_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:33.36 +41:25:22.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31519_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31519_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:45.70 +40:57:32.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31523_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31523_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:30.40 +41:02:39.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31524_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31524_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:47.06 +41:48:00.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31526_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31526_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:45.28 +42:01:05.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31529_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31529_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:24.45 +41:16:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.01, MAG_FAINT_SEARCH_LIMIT=9.99)GAIADR2_OUTPUT=# 1.738 194894006600026496 080.10160668215 +41.28117250013 8.4467 7.3690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31533_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31533_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:49.88 +41:30:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.18, MAG_FAINT_SEARCH_LIMIT=10.16)GAIADR2_OUTPUT=# 1.476 195089062536158208 079.45739984689 +41.50269485485 8.8706 8.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31534_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31534_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:56.67 +42:14:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.18, MAG_FAINT_SEARCH_LIMIT=10.16)GAIADR2_OUTPUT=# 1.503 207181117761067520 079.23564979016 +42.24980842582 8.8038 7.8874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31542_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31542_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:52.90 +42:07:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.45, MAG_FAINT_SEARCH_LIMIT=10.43)GAIADR2_OUTPUT=# 1.275 207176582275392896 079.22057342903 +42.12461002990 9.3696 9.2723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31543_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31543_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:49.64 +41:27:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.49, MAG_FAINT_SEARCH_LIMIT=10.47)GAIADR2_OUTPUT=# 0.778 194910804216589568 079.95683514461 +41.46502160365 9.1602 8.2861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31544_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31544_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:12.97 +41:03:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.47, MAG_FAINT_SEARCH_LIMIT=10.45)GAIADR2_OUTPUT=# 2.492 194874902585663104 079.55417862473 +41.05531547706 9.1834 8.4693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31545_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31545_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:10.97 +41:02:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.51, MAG_FAINT_SEARCH_LIMIT=10.49)GAIADR2_OUTPUT=# 1.764 194838859220341504 080.29586036541 +41.04724591507 9.2725 8.5890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31547_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31547_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:50.19 +41:52:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.58, MAG_FAINT_SEARCH_LIMIT=10.56)GAIADR2_OUTPUT=# 1.005 195168059873633152 079.45940082078 +41.86775544405 9.4742 9.3025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31549_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31549_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:31.05 +41:40:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.55, MAG_FAINT_SEARCH_LIMIT=10.53)GAIADR2_OUTPUT=# 1.843 195094800612459648 079.37871873225 +41.66889798060 8.9243 7.7659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31553_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31553_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:22.58 +40:58:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.62, MAG_FAINT_SEARCH_LIMIT=10.60)GAIADR2_OUTPUT=# 3.828 194829479011707136 080.59455393543 +40.97410899316 9.5500 9.4659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31557_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31557_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:53.16 +41:10:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.72, MAG_FAINT_SEARCH_LIMIT=10.70)GAIADR2_OUTPUT=# 0.222 194844249402122368 080.47158143004 +41.17132691307 9.5100 8.8233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31559_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31559_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:46.26 +41:22:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.77, MAG_FAINT_SEARCH_LIMIT=10.75)GAIADR2_OUTPUT=# 1.889 195070890533769216 079.44273683908 +41.38172530938 9.4354 8.6008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31563_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31563_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:25.35 +42:13:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.83, MAG_FAINT_SEARCH_LIMIT=10.81)GAIADR2_OUTPUT=# 0.979 207177578707741312 079.35593769974 +42.23188514755 9.7134 9.6708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31569_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31569_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:49.71 +42:00:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.01, MAG_FAINT_SEARCH_LIMIT=10.99)GAIADR2_OUTPUT=# 0.532 195164074139590144 079.20719309813 +42.01269436599 9.7853 9.1047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31578_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31578_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:47.62 +40:57:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.03, MAG_FAINT_SEARCH_LIMIT=11.01)GAIADR2_OUTPUT=# 2.184 194861841587237888 079.94893452378 +40.95736965217 9.9283 9.8117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31582_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31582_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:40.12 +41:14:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.03, MAG_FAINT_SEARCH_LIMIT=11.01)GAIADR2_OUTPUT=# 1.370 194880670724788736 079.91715800677 +41.23948053120 9.7124 8.8411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31586_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31586_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:11.83 +40:58:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.10, MAG_FAINT_SEARCH_LIMIT=11.08)GAIADR2_OUTPUT=# 2.448 194835457606280320 080.29989299046 +40.97060488817 10.0084 9.9393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31588_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31588_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:22.70 +41:56:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 0.947 195168712708586880 079.59481807730 +41.93499779019 10.0610 9.6821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31589_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31589_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:14:59.12 +46:47:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31593_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31593_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:28.49 +40:55:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 2.349 194834422516027648 080.36927441734 +40.92417388810 10.2011 9.9570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31595_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31595_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:13.64 +40:59:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 2.816 194859715581278976 079.80671011876 +40.98633445397 9.9252 8.9281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31598_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31598_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:52.34 +40:57:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)GAIADR2_OUTPUT=# 2.517 194871054294960000 079.71841581503 +40.96370847087 10.1244 9.4454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31600_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31600_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:55.78 +41:11:56.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)
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Considering the candidate 31601_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31601_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:49.12 +41:46:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 1.330 195108170849542656 079.95417197636 +41.76770633339 9.7038 8.5210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31604_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31604_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:37.71 +41:12:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 1.393 194880464565429888 079.90732705922 +41.20217200222 10.1470 9.4366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31607_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31607_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:00.57 +41:30:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 1.360 195098756281722880 079.75258099041 +41.51495586338 10.1418 9.4703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31609_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31609_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:41.55 +41:21:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 1.159 194908399033652480 079.92327243680 +41.35511431619 10.2237 9.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31614_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31614_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:11.13 +41:47:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 1.129 195119848861724160 079.54647313629 +41.79288962471 10.1726 9.3474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31618_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31618_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:37.57 +41:21:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 1.375 194908437690158080 079.90696571114 +41.36053871552 10.4726 10.1839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31619_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31619_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:41.59 +41:18:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 1.064 194893663002624256 080.17337041007 +41.30098806369 10.2689 9.4462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31624_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31624_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:59.71 +41:36:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 1.583 195135486838560256 079.24875864978 +41.60491112853 10.4053 9.7473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31625_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31625_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:43.84 +41:02:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 1.937 194865316219023744 079.93319963446 +41.04297553053 10.4777 10.4030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31629_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31629_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:35.28 +41:30:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 1.374 195089960188513152 079.39718452152 +41.51107808745 10.5330 10.2994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31639_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31639_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:04.61 +41:49:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 1.101 195146516317751296 079.26957255562 +41.83221984535 10.7035 10.4112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31640_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31640_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:58.68 +41:54:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 0.882 195169021946272512 079.49473635738 +41.91341265179 10.7258 10.6123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31641_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31641_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:09.74 +40:56:38.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)
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Considering the candidate 31642_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31642_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:36.29 +41:57:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 0.721 195170121457832448 079.65109474893 +41.95312384409 10.6270 9.9277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31645_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31645_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:36.05 +41:00:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 3.654 194829822609056000 080.65022774721 +41.00431846505 10.3793 9.3680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31649_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31649_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:25.61 +40:56:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 2.461 194858650429865472 079.85730286787 +40.94390115231 10.6999 10.3853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31655_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31655_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:34.15 +41:32:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 0.668 194914347565063040 080.14217400966 +41.53691326445 10.9132 10.7015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31656_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31656_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:09.53 +41:39:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 1.558 195104253839474432 079.79006675695 +41.66047878957 10.7953 10.7051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31669_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31669_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:32.80 +41:37:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 1.396 195101195823129984 079.88689469049 +41.62815393624 10.7825 10.2635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31674_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31674_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:08.97 +41:35:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 1.066 195088444060864896 079.28711088270 +41.58758165967 10.7259 9.9311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31689_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31689_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:00.04 +41:48:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 0.924 195120540355488256 079.50044511101 +41.80184898559 10.8767 10.4066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31691_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31691_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:17.12 +41:01:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.164 194865728535472768 079.82189491218 +41.03237903708 10.9511 10.8634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31698_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31698_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:12.42 +41:07:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.828 194879094473677824 079.80194359823 +41.11818033204 10.7622 9.9860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31706_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31706_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:35.67 +40:54:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 3.776 188868923400429696 079.39880485125 +40.90409882667 10.7451 9.9034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31709_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31709_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:43.67 +41:05:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.264 195063400111019392 079.43244735006 +41.09518492146 10.9951 10.7180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31711_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31711_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:36.24 +41:26:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.145 194912694000958848 080.15140226917 +41.43665658075 11.1162 10.9503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31715_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31715_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:59.11 +40:55:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.430 194860746373868672 079.99684804615 +40.91913865447 11.0057 10.6815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31729_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31729_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:26.75 +41:09:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 0.607 194841882877244800 080.36157555147 +41.16194911802 11.1781 10.8951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31734_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31734_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:27.05 +42:04:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.345 195163245211271168 079.36307125590 +42.07876882175 11.0301 10.8680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31735_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31735_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:00.71 +41:37:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.101 195102776370750592 079.75295790949 +41.63347243684 10.9001 10.1009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31736_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31736_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:09.94 +40:54:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 2.257 194834770411547008 080.29183928375 +40.91537706964 11.1522 10.8767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31737_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31737_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:19.26 +40:58:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 2.305 194835522027653632 080.33071579898 +40.97243708222 11.0787 10.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31753_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31753_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:02.20 +41:10:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.772 194882393004730880 079.75942439727 +41.17593643605 10.9554 10.2867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31757_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31757_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:32.68 +41:34:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 2.140 195100027592029568 079.88673925015 +41.57927340442 11.1915 10.9744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31762_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31762_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:17:39.37 +41:49:49.3: 12.85 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:17:39.37 +41:49:49.3: 10.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.01
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Considering the candidate 31763_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31763_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:44.90 +41:25:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 1.237 194909193604376448 079.93741409759 +41.42445654682 11.1301 10.7233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31775_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31775_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:49.72 +41:51:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 1.143 195118753649002496 079.70714522513 +41.85076634070 10.9044 10.0128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31777_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31777_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:09.93 +41:28:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.971 194911014670478336 080.04161239436 +41.48234153419 11.1962 10.4901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31788_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31788_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:16.46 +41:57:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.973 195161291005178112 079.31846835127 +41.95985478282 11.0678 10.3464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31789_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31789_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:52.19 +41:10:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.543 194882255569609472 079.71752157523 +41.16826853933 11.0008 10.2720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31790_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31790_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:21.40 +41:38:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 1.049 195101157166086016 079.83924140263 +41.64659157681 11.1014 10.3993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31792_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31792_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:32.68 +41:00:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 2.808 189057455283431680 079.38668216873 +41.00807408205 11.1228 10.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31795_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31795_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:04.50 +41:02:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 2.511 194842295194111232 080.51926640292 +41.03847710758 11.1142 10.6361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31798_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31798_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:00.21 +41:05:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 3.051 195062815995460096 079.50100027594 +41.09421334560 11.3584 11.0832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31799_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31799_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:30.33 +41:50:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 1.065 195145240708375296 079.37655920881 +41.83726581411 11.0491 10.3387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31800_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31800_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:31.24 +41:15:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.221 194881598437726336 079.88044539143 +41.26264993183 11.2162 10.7295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31804_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31804_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:26.45 +41:33:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 2.052 195099890153078912 079.86066034273 +41.56145898197 11.2580 11.1331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31806_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31806_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:17.31 +41:44:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.444 195142388850095744 079.32223862782 +41.74524674223 11.0454 10.3594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31812_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31812_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:34.12 +40:54:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.920 194814944842570880 080.14259938579 +40.90818973441 11.1869 10.4867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31823_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31823_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:01.34 +41:28:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 1.408 195098515763704960 079.75573862339 +41.48229005413 11.1538 10.4416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31836_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31836_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:47.66 +41:19:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 1.431 194850331075823104 080.44876111698 +41.32248538757 11.3441 11.0207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31840_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 31840_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:57.31 +41:19:29.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)
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Considering the candidate 04959_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 04959_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:46:08.74 +47:54:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 2.584 966719627056755456 101.53555420829 +47.90075880365 10.9650 10.6141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 16670_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 16670_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:26:01.78 +50:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:41:12.85 +44:09:59.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 24s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:27:04.73 +50:07:23.2
05:18:28.49 +43:23:12.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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
Plate-solving the images
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 935.1'x631.3' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 05:59:47.823 +46:00:35.63 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:47.028 +45:55:19.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 05:59:47.028 +45:55:19.19
Angular distance between the image centers 0.0879 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:47.731 +45:56:00.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 05:59:47.731 +45:56:00.01
Angular distance between the image centers 0.0766 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:59:47.028 +45:55:19.19
Second-epoch second image center 05:59:47.731 +45:56:00.01
Angular distance between the image centers 0.01152 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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.5wET2mbtFX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.vwk98JB8j2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits &> /tmp/tmp.AfTCkYsq6f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits &> /tmp/tmp.TPvOYoJ3xp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 170851 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.8948 to 102.5178 deg, Dec +39.9772 to +51.3479 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 77.8948 to 102.5178 deg, Dec 39.9772 to 51.3479 deg
Loaded 11844 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): 101 out of 140 total matches.
Matched with Tycho-2 140 out of 170851 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.801794
a=0.000000 b=1.000000 c=21.801794
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 170851 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.8948 to 102.5178 deg, Dec +39.9772 to +51.3479 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 77.8948 to 102.5178 deg, Dec 39.9772 to 51.3479 deg
Loaded 11844 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): 101 out of 140 total matches.
Matched with Tycho-2 140 out of 170851 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (aperture=4.6)
Read 170104 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.8829 to 102.6552 deg, Dec +39.9573 to +51.3529 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 77.8829 to 102.6552 deg, Dec 39.9573 to 51.3529 deg
Loaded 11951 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): 6467 out of 8981 total matches.
Matched with Tycho-2 8981 out of 170104 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 602 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
2.0 pix wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
13.2 mag. fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
13.2 mag. fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
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.5wET2mbtFX (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=20120, passed=170805
Got 170805 stars (including 150422 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 170805 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 406 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 356 matched stars entering correct_measured_positions(), 310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.13"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 60456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.06"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 442 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 410 matched stars entering correct_measured_positions(), 60493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.05"
Accuracy estimation diagnostic: 409 matched stars entering correct_measured_positions(), 73193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.14"
Excluding outliers - 409 stars left (next iteration limit 387)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.vwk98JB8j2 (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=20075, passed=170053
Got 170053 stars (including 149705 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170053 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.AfTCkYsq6f (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=3837, passed=73915
Got 73915 stars (including 69944 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat
util/solve_plate_with_UCAC5 got 73915 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 72625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 72626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 72617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 930 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.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.TPvOYoJ3xp (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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.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_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=3619, passed=72175
Got 72175 stars (including 68445 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 72175 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 70591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 648 to 708 (Dec 39.7 to 51.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 70595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 70604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 927 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.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_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-33-08_20.00sec_-4.90C_LIGHTs_0019.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Aur-02-Q1b1x1_233522_TTUQ1b1x1_3506432_iwhJAgLq/wcs_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out132003.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out196406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out111171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68332.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 366s
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: 160s
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Considering the candidate 195165_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195165_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:53:28.96 +46:52:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.370 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195172_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195172_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:49:53.97 +47:59:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195173_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195173_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:56:29.64 +45:53:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.779 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195177_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195177_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195184_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195184_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:44:07.42 +49:44:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.772 991132908361397376 101.03160541176 +49.74457142885 13.6325 13.1029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195187_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195187_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:36:55.33 +50:56:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195192_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195192_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:23:15.09 +41:57:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195193_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195193_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:57:24.91 +48:02:36.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 195195_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195195_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:27:54.89 +49:56:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195198_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195198_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195200_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195200_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 195201_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195201_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:32:39.67 +41:07:20.5: 12.27 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:32:39.67 +41:07:20.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
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Considering the candidate 195202_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195202_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:27:16.19 +45:33:31.9: 12.23 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:27:16.19 +45:33:31.9: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.03
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Considering the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195206_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195206_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:53.53 +42:28:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195207_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195207_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195208_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195208_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195209_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195209_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:26.19 +42:20:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.768 195228769233053952 080.35976775845 +42.33526266838 13.0244 12.1265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195211_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195211_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:24:58.83 +40:59:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195217_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195217_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195218_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195218_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:25:09.84 +41:59:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 2.913 194988044904843264 081.29164698377 +41.98676172731 12.8172 11.7924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195219_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195219_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:42:01.78 +46:28:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.300 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195221_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195221_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195223_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195223_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:03:22.98 +42:40:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195224_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195224_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:41.70 +42:50:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.993 207312956076563200 080.17406803057 +42.84273080140 12.8468 12.2799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195225_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195225_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:38.50 +43:03:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.419 207295428310390272 079.41043476881 +43.05402273547 12.7873 11.7607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195226_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195226_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:23:13.12 +41:14:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 2.681 194927644784632576 080.80446133462 +41.24995087291 13.0007 12.1111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195227_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195227_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195231_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195231_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:24:58.00 +42:35:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195233_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:00.08 +43:23:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195235_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195235_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:35:48.36 +41:58:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195236_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195236_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:43.12 +41:31:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.611 194947264195158016 080.67986339367 +41.52997321366 12.6549 11.7735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195240_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195240_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195241_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195241_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:25:19.64 +40:59:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195242_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195242_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:23:44.30 +42:29:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 1.491 195246056479667072 080.93483733021 +42.49723041978 12.6429 11.6008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195243_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195243_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195245_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195245_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:24:47.81 +43:12:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195248_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195248_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:51:38.23 +48:20:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 0.989 210370418736729472 087.90946632657 +48.33580450234 12.7164 12.1774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195249_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195249_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:25:35.61 +49:58:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195250_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195250_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:28.61 +42:15:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 2.824 195273475551645952 080.12022708554 +42.26410525122 12.3502 11.3310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195252_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195252_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195254_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195254_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195256_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195256_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:57:46.11 +43:34:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195257_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195257_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:26:48.16 +43:44:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195258_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195258_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195259_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195259_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195260_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195260_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:48:07.47 +45:19:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 0.734 197617561323923584 087.03135150238 +45.31853933119 12.1463 11.6118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195261_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195261_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:57:08.99 +46:13:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.087 197771561669756288 089.28789413872 +46.22871042011 12.0773 11.6194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195264_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195264_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:46:10.50 +47:53:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195266_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195266_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195268_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195268_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:28:11.13 +45:21:58.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)
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Considering the candidate 195269_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195269_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:02.59 +42:11:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195270_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195270_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:14.60 +41:05:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195271_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195271_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:55.48 +41:05:46.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195279_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195279_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:23.91 +42:06:37.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195280_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195280_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:40.61 +41:13:13.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195282_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195282_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:49:28.76 +49:41:31.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195283_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195283_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:55.35 +40:59:01.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195284_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195284_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:51.20 +41:14:30.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195285_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195285_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:33.40 +41:25:20.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195288_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195288_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:45.71 +40:57:31.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195292_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195292_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:30.39 +41:02:38.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195293_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195293_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:47.04 +41:48:02.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195295_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195295_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:45.26 +42:01:06.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 195297_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195297_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:24.45 +41:16:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 7.96, MAG_FAINT_SEARCH_LIMIT=8.94)GAIADR2_OUTPUT=# 1.738 194894006600026496 080.10160668215 +41.28117250013 8.4467 7.3690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195301_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195301_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:49.87 +41:30:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.11, MAG_FAINT_SEARCH_LIMIT=9.09)GAIADR2_OUTPUT=# 1.216 195089062536158208 079.45739984689 +41.50269485485 8.8706 8.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195303_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195303_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:56.68 +42:14:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.12, MAG_FAINT_SEARCH_LIMIT=9.10)GAIADR2_OUTPUT=# 1.550 207181117761067520 079.23564979016 +42.24980842582 8.8038 7.8874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195308_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195308_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:01.35 +41:41:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.27, MAG_FAINT_SEARCH_LIMIT=9.25)GAIADR2_OUTPUT=# 1.076 195106968259164800 080.00578508159 +41.69905166754 9.2406 8.8718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195312_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195312_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195313_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:49.64 +41:27:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.41, MAG_FAINT_SEARCH_LIMIT=9.39)GAIADR2_OUTPUT=# 0.578 194910804216589568 079.95683514461 +41.46502160365 9.1602 8.2861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195314_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195314_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:12.98 +41:03:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.38, MAG_FAINT_SEARCH_LIMIT=9.36)GAIADR2_OUTPUT=# 2.577 194874902585663104 079.55417862473 +41.05531547706 9.1834 8.4693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195315_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:10.97 +41:02:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.42, MAG_FAINT_SEARCH_LIMIT=9.40)GAIADR2_OUTPUT=# 1.570 194838859220341504 080.29586036541 +41.04724591507 9.2725 8.5890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195317_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195317_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195322_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195322_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:22.58 +40:58:29.3: 8.71 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:22.58 +40:58:29.3: 9.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.18 +/- 0.00
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Considering the candidate 195323_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195323_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:31.06 +41:40:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.51, MAG_FAINT_SEARCH_LIMIT=9.49)GAIADR2_OUTPUT=# 1.884 195094800612459648 079.37871873225 +41.66889798060 8.9243 7.7659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195325_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195325_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:53.18 +41:10:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.64, MAG_FAINT_SEARCH_LIMIT=9.62)GAIADR2_OUTPUT=# 1.477 194844249402122368 080.47158143004 +41.17132691307 9.5100 8.8233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195329_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195329_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:46.30 +41:22:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.69, MAG_FAINT_SEARCH_LIMIT=9.67)GAIADR2_OUTPUT=# 0.861 195070890533769216 079.44273683908 +41.38172530938 9.4354 8.6008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195333_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195333_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:25.33 +42:13:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.74, MAG_FAINT_SEARCH_LIMIT=9.72)GAIADR2_OUTPUT=# 2.273 207177578707741312 079.35593769974 +42.23188514755 9.7134 9.6708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195344_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195344_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:49.70 +42:00:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.94, MAG_FAINT_SEARCH_LIMIT=9.92)GAIADR2_OUTPUT=# 2.319 195164074139590144 079.20719309813 +42.01269436599 9.7853 9.1047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195346_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195346_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195352_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195352_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:40.12 +41:14:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.95, MAG_FAINT_SEARCH_LIMIT=9.93)GAIADR2_OUTPUT=# 1.270 194880670724788736 079.91715800677 +41.23948053120 9.7124 8.8411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195357_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195357_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195359_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195359_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:22.68 +41:56:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.10, MAG_FAINT_SEARCH_LIMIT=10.08)GAIADR2_OUTPUT=# 2.089 195168712708586880 079.59481807730 +41.93499779019 10.0610 9.6821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195363_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195363_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:28.50 +40:55:28.3: 9.61 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:28.50 +40:55:28.3: 10.27 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.05 +/- 0.00
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Considering the candidate 195364_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195364_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:03.33 +41:14:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.23, MAG_FAINT_SEARCH_LIMIT=10.21)GAIADR2_OUTPUT=# 1.137 194848887966800768 080.51383753532 +41.23734230408 9.9358 9.0096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195367_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195367_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:13.66 +40:59:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.25, MAG_FAINT_SEARCH_LIMIT=10.23)GAIADR2_OUTPUT=# 2.656 194859715581278976 079.80671011876 +40.98633445397 9.9252 8.9281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195368_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195368_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:52.36 +40:57:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.27, MAG_FAINT_SEARCH_LIMIT=10.25)GAIADR2_OUTPUT=# 2.159 194871054294960000 079.71841581503 +40.96370847087 10.1244 9.4454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195373_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195373_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:49.13 +41:46:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.32, MAG_FAINT_SEARCH_LIMIT=10.30)GAIADR2_OUTPUT=# 1.463 195108170849542656 079.95417197636 +41.76770633339 9.7038 8.5210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195374_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195374_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:37.72 +41:12:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.32, MAG_FAINT_SEARCH_LIMIT=10.30)GAIADR2_OUTPUT=# 1.258 194880464565429888 079.90732705922 +41.20217200222 10.1470 9.4366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195376_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195376_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:00.58 +41:30:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.29, MAG_FAINT_SEARCH_LIMIT=10.27)GAIADR2_OUTPUT=# 1.040 195098756281722880 079.75258099041 +41.51495586338 10.1418 9.4703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195378_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195378_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:41.55 +41:21:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.36, MAG_FAINT_SEARCH_LIMIT=10.34)GAIADR2_OUTPUT=# 1.066 194908399033652480 079.92327243680 +41.35511431619 10.2237 9.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195381_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195381_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:11.18 +41:47:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.40, MAG_FAINT_SEARCH_LIMIT=10.38)GAIADR2_OUTPUT=# 0.500 195119848861724160 079.54647313629 +41.79288962471 10.1726 9.3474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195388_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195388_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195390_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195390_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:41.59 +41:18:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.48, MAG_FAINT_SEARCH_LIMIT=10.46)GAIADR2_OUTPUT=# 0.217 194893663002624256 080.17337041007 +41.30098806369 10.2689 9.4462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195394_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:43.85 +41:02:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.52, MAG_FAINT_SEARCH_LIMIT=10.50)GAIADR2_OUTPUT=# 1.721 194865316219023744 079.93319963446 +41.04297553053 10.4777 10.4030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195395_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195395_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:59.72 +41:36:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.54, MAG_FAINT_SEARCH_LIMIT=10.52)GAIADR2_OUTPUT=# 0.903 195135486838560256 079.24875864978 +41.60491112853 10.4053 9.7473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195397_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195397_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195400_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:35.25 +41:30:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.58, MAG_FAINT_SEARCH_LIMIT=10.56)GAIADR2_OUTPUT=# 1.446 195089960188513152 079.39718452152 +41.51107808745 10.5330 10.2994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195413_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195413_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:36.27 +41:57:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.70, MAG_FAINT_SEARCH_LIMIT=10.68)GAIADR2_OUTPUT=# 1.656 195170121457832448 079.65109474893 +41.95312384409 10.6270 9.9277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195416_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195416_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:36.05 +41:00:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.73, MAG_FAINT_SEARCH_LIMIT=10.71)GAIADR2_OUTPUT=# 3.154 194829822609056000 080.65022774721 +41.00431846505 10.3793 9.3680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195420_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:25.63 +40:56:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.72, MAG_FAINT_SEARCH_LIMIT=10.70)GAIADR2_OUTPUT=# 2.086 194858650429865472 079.85730286787 +40.94390115231 10.6999 10.3853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195423_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195423_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195424_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195424_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195434_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195434_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:59:43.42 +44:59:09.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 195440_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195440_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:08.96 +41:35:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.87, MAG_FAINT_SEARCH_LIMIT=10.85)GAIADR2_OUTPUT=# 0.667 195088444060864896 079.28711088270 +41.58758165967 10.7259 9.9311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195447_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195447_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:00.03 +41:48:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.93, MAG_FAINT_SEARCH_LIMIT=10.91)GAIADR2_OUTPUT=# 2.496 195120540355488256 079.50044511101 +41.80184898559 10.8767 10.4066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195449_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195449_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195451_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195451_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:12.43 +41:07:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.93, MAG_FAINT_SEARCH_LIMIT=10.91)GAIADR2_OUTPUT=# 1.605 194879094473677824 079.80194359823 +41.11818033204 10.7622 9.9860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195458_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195458_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:35.70 +40:54:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.97, MAG_FAINT_SEARCH_LIMIT=10.95)GAIADR2_OUTPUT=# 3.248 188868923400429696 079.39880485125 +40.90409882667 10.7451 9.9034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195468_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195468_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195469_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195469_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:08.98 +41:46:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.01, MAG_FAINT_SEARCH_LIMIT=10.99)GAIADR2_OUTPUT=# 0.894 195119818800980992 079.53755781599 +41.78161391557 10.9528 10.5173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195471_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195471_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195472_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195472_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:00.72 +41:37:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.03, MAG_FAINT_SEARCH_LIMIT=11.01)GAIADR2_OUTPUT=# 0.710 195102776370750592 079.75295790949 +41.63347243684 10.9001 10.1009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195473_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195473_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195478_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195478_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195482_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195482_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:09.95 +40:54:56.8: 10.47 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:09.95 +40:54:56.8: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
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Considering the candidate 195484_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195484_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:02.21 +41:10:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.08, MAG_FAINT_SEARCH_LIMIT=11.06)GAIADR2_OUTPUT=# 1.544 194882393004730880 079.75942439727 +41.17593643605 10.9554 10.2867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195492_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195492_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:49.72 +41:51:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.15, MAG_FAINT_SEARCH_LIMIT=11.13)GAIADR2_OUTPUT=# 0.169 195118753649002496 079.70714522513 +41.85076634070 10.9044 10.0128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195494_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195494_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195496_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195496_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195506_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195506_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:16.44 +41:57:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 2.424 195161291005178112 079.31846835127 +41.95985478282 11.0678 10.3464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195509_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195509_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:52.20 +41:10:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.19, MAG_FAINT_SEARCH_LIMIT=11.17)GAIADR2_OUTPUT=# 1.335 194882255569609472 079.71752157523 +41.16826853933 11.0008 10.2720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195511_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195511_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:32.71 +41:00:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 2.293 189057455283431680 079.38668216873 +41.00807408205 11.1228 10.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195512_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195512_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:04.59 +41:02:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 1.565 194842295194111232 080.51926640292 +41.03847710758 11.1142 10.6361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195514_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195514_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:21.40 +41:38:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 1.049 195101157166086016 079.83924140263 +41.64659157681 11.1014 10.3993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195515_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195515_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:30.31 +41:50:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 2.932 195145240708375296 079.37655920881 +41.83726581411 11.0491 10.3387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195517_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195517_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195521_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195521_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:17.29 +41:44:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 3.354 195142388850095744 079.32223862782 +41.74524674223 11.0454 10.3594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195522_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195522_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:16.55 +42:16:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 2.054 195192283488673920 079.56893777489 +42.27179084549 11.0719 10.2511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195525_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195525_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195526_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195526_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195531_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195531_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195536_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195536_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:34.14 +40:54:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 1.544 194814944842570880 080.14259938579 +40.90818973441 11.1869 10.4867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195539_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195539_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195541_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195541_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:27.10 +41:08:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.23, MAG_FAINT_SEARCH_LIMIT=11.21)GAIADR2_OUTPUT=# 1.066 194841092603273088 080.36311506649 +41.14021659222 11.1327 10.4341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195545_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195545_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:01.34 +41:28:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 0.854 195098515763704960 079.75573862339 +41.48229005413 11.1538 10.4416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195555_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195555_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195557_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195557_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:07.33 +41:03:41.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195561_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195561_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195563_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195563_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195565_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195565_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195566_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195566_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195567_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195567_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195568_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195568_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:10.41 +40:56:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.35, MAG_FAINT_SEARCH_LIMIT=11.33)GAIADR2_OUTPUT=# 2.279 194860849453052800 080.04391272513 +40.94012552697 11.2920 10.7363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195572_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195572_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195574_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195574_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195576_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195576_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:11.24 +41:39:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 0.943 195141461137164288 079.29691797538 +41.65069857682 11.3044 10.8770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195577_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195577_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195578_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195578_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:29.02 +41:34:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 0.876 195079613608105216 079.62091090687 +41.57016007991 11.2093 10.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195581_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195581_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:08.43 +41:30:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 0.734 195089272993695744 079.53519627180 +41.51244668128 11.2362 10.5224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195586_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195586_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:07.69 +41:52:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 0.634 195119028526877056 079.78216824955 +41.86703775995 11.2840 10.5487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195594_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195594_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195597_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195597_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:26.44 +41:22:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 1.271 195072986478103424 079.61036245720 +41.36690115203 11.1862 10.4492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195598_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195598_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195599_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195599_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195601_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195601_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:10.00 +42:25:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.44, MAG_FAINT_SEARCH_LIMIT=11.42)GAIADR2_OUTPUT=# 2.912 207195132234117760 079.29150998962 +42.42303277669 11.2938 10.5227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195607_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195607_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:27.23 +41:26:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 1.317 194909777719941376 079.86383808223 +41.43470193372 11.3637 10.6593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195608_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195608_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:57.68 +41:18:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.44, MAG_FAINT_SEARCH_LIMIT=11.42)GAIADR2_OUTPUT=# 1.100 194893559923393152 080.24071931485 +41.31079245616 11.3941 10.7140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195615_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195615_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:13.24 +41:15:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 1.466 194892597850768768 080.05569357314 +41.26468363197 11.4298 10.8482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195617_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195617_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:12.02 +41:25:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)GAIADR2_OUTPUT=# 0.793 195083427538537600 079.29980378229 +41.43009583137 11.1391 10.1546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195619_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195619_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:00.94 +41:30:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 1.202 194911250893192576 080.00422477466 +41.50510252198 11.4232 10.9252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195621_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195621_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195622_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195622_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:53.43 +41:52:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 2.588 195147856347539456 079.22306850405 +41.88091703689 11.4877 11.0935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195625_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195625_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:01.98 +42:07:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 1.865 195186236175090176 079.50826808495 +42.11800987720 11.4607 10.7004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195626_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195626_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:39.61 +40:57:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)GAIADR2_OUTPUT=# 2.186 194864388506141952 079.91510846491 +40.96322827020 11.4195 10.6521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195629_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195629_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:23:09.69 +40:56:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 3.096 194827005110492928 080.79056749215 +40.94490240215 11.3140 10.5254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195632_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195632_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195634_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195634_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195637_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195637_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195642_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195642_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195644_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195644_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195646_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195646_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195648_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195648_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195652_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195652_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:26.70 +41:48:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 0.768 195111847341563264 079.86149355040 +41.80166756858 11.6595 11.1972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195654_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195654_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:30.25 +41:17:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 0.705 194894075319493760 080.12626517650 +41.29831594132 11.5380 10.7215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195666_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195666_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:19.58 +41:22:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.67, MAG_FAINT_SEARCH_LIMIT=11.65)GAIADR2_OUTPUT=# 0.809 194897094679740928 080.33165433955 +41.37585713473 11.4483 10.5686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195668_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195668_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:45:42.92 +43:37:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195672_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195672_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195675_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195675_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:45.50 +41:28:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 1.596 194911564426308096 079.93989906025 +41.48329148497 11.6072 11.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195676_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195676_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195679_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195679_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195685_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195685_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195688_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195688_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:57.26 +42:03:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 3.320 195165787831910912 079.23876772741 +42.05069911115 11.6323 10.9095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195694_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195694_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:11:34.54 +48:44:35.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195696_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195696_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195700_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195700_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195703_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195703_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:16.40 +40:58:15.7: 10.91 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:16.40 +40:58:15.7: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.01
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Considering the candidate 195704_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195704_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:54.25 +40:59:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 3.655 194828035902644480 080.72613107801 +40.98973694046 11.4691 10.4099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195706_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195706_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195709_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195709_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195710_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195710_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195712_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195712_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:59.91 +42:19:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.892 207182316051712640 079.24952861101 +42.31825525503 11.6669 10.8093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195713_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195713_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195715_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195715_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195716_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195716_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:32.76 +41:36:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 0.602 195100817866009472 079.88663113948 +41.60802434766 11.7339 11.0045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195724_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195724_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195725_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195725_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:28.43 +41:10:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 1.568 194877200390718208 079.61837624882 +41.16784670833 11.7232 10.9122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195729_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195729_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195731_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195731_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:28.07 +41:06:58.2: 11.42 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:28.07 +41:06:58.2: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
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Considering the candidate 195733_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195733_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195736_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195736_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:27:49.82 +48:14:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 0.932 212658742954328448 081.95741015715 +48.24842633959 11.8385 11.0011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195737_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195737_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:47.34 +41:17:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 0.570 194904963059815936 079.94739803007 +41.29885964027 11.8562 11.0543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195739_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195739_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:32.00 +42:10:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 2.147 195190870447427584 079.38376112515 +42.18046699810 11.8365 11.0377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195740_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195740_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:27.78 +41:58:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 2.814 195149952291490688 079.36550877399 +41.97754482328 11.5173 10.4121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195747_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195747_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195749_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195749_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195751_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195751_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195752_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195752_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195754_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195754_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:03.01 +41:14:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 0.740 194892215596882432 080.01261232398 +41.24294034451 11.8421 11.0671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195755_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195755_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195757_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195757_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195758_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195758_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195763_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195763_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:34.77 +41:08:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 1.628 194877032889398272 079.64519417674 +41.14908914525 11.8517 11.4438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195768_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195768_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:48.69 +41:19:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 1.222 195071676508547456 079.70303553824 +41.31718268242 11.9907 11.2357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195771_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195771_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195772_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195772_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195776_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195776_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:00.03 +40:57:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195779_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195779_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:10.74 +41:00:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 2.023 194873558258453120 079.54496507465 +41.00668426591 11.9286 11.2631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195780_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195780_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:09.37 +41:56:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 2.146 195169399903373184 079.53926053879 +41.93317665164 11.8295 11.0534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195782_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195782_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195784_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195784_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 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 195787_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195787_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:09.11 +42:24:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 2.955 207195132234118528 079.28775770447 +42.41391483068 11.6473 10.5554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195789_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195789_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:43:31.71 +50:41:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 3.585 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195791_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195791_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195794_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195794_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195803_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195803_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:46.26 +41:30:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 0.540 194913484274940800 080.19287206201 +41.50292463418 11.9517 11.0739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195808_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195808_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195811_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195811_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:24.87 +40:53:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.833 194869778687234816 079.60387491570 +40.89136050215 12.0643 11.4635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195818_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195818_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:19.74 +41:29:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.582 195098167868886528 079.83265402573 +41.49515205986 12.0962 11.5050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195819_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195819_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195821_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195821_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195834_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195834_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195836_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195836_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:44.52 +40:57:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 3.576 188869438796491008 079.43536808773 +40.95956722929 11.8976 10.8872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195839_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195839_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:43.65 +41:17:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.145 194905001716339072 079.93220468569 +41.28321733380 12.1349 11.4386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195848_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195848_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195849_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195849_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195850_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195850_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195852_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195852_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:01.49 +41:06:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195854_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195854_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:13.48 +41:57:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 2.412 195169567403134208 079.55658504866 +41.95587892051 12.1224 11.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195858_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195858_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:17.08 +41:45:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 0.760 195119509563338752 079.57109937689 +41.75142732667 12.1520 11.3541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195859_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195859_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:34.73 +41:03:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 1.413 194875448044062848 079.64473748780 +41.05891359472 11.9858 11.1586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195864_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195864_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:08.18 +41:27:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195865_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195865_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195866_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195866_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:59:57.61 +45:53:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195867_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195867_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:56.67 +41:17:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.473 194904275865048832 079.98666954085 +41.28439399939 12.2469 11.7517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195869_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195869_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:28.64 +41:18:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195870_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195870_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:28.85 +41:54:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 3.057 195148779761424128 079.37014740396 +41.90723527321 11.9341 11.0181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195871_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195871_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:06:21.27 +48:46:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.668 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195874_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195874_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195882_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195882_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195888_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195888_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195898_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195898_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:13.00 +41:07:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195900_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195900_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:47.04 +41:52:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.136 195168880209495808 079.44450434951 +41.87960615542 12.2191 11.3594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195901_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195901_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:49.99 +41:55:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 2.419 195169189452387072 079.45819314394 +41.92502640143 12.1029 11.2369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195905_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195905_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195906_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195906_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195908_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195908_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:11.45 +41:38:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.192 195141461137164672 079.29788974892 +41.64130199960 12.2466 11.7871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195909_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195909_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:40.15 +41:17:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.081 195071573428801664 079.66758378689 +41.29201724933 12.2677 11.7724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195913_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195913_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:09.16 +41:58:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 2.490 195169739201825408 079.53837701608 +41.97232613558 12.2382 11.7344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195914_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195914_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195922_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195922_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:33.10 +40:59:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 2.645 189057249125003776 079.38842459625 +40.98901219187 12.2338 11.6503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195926_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195926_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195927_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195927_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:11.33 +41:17:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.718 194896166966807040 080.29750146886 +41.29347886410 12.3811 11.8828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195930_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195930_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195932_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195932_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:31.21 +41:03:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 1.835 194875344964847872 079.63046871530 +41.05785496416 12.2651 11.8289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195934_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195934_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195936_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195936_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195937_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195937_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195940_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195940_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195943_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195943_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195946_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195946_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:28.06 +41:25:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.412 194898743947181824 080.36698355528 +41.42432508068 12.2079 11.2911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195949_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195949_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:19.58 +41:06:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.807 194876444476474752 079.58178701136 +41.10666098507 12.2272 11.3968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195951_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195951_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:19:04.24 +47:21:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.229 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195953_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195953_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195959_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195959_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195967_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195967_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195972_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195972_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:36.21 +41:39:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.068 195115180236316928 079.65089597496 +41.66693513721 12.2969 11.4923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195977_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195977_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:18.20 +41:03:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.850 189058241257287040 079.32553102671 +41.05810295483 12.0767 11.0339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195979_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195979_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:26.31 +41:21:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.469 194908570833596672 079.85973338649 +41.35962791542 12.3031 11.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195980_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195980_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:33.88 +41:06:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 1.315 194840817725370112 080.39109492266 +41.11130579227 12.1509 11.1759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195981_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195981_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195982_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195982_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 195985_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195985_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:32.06 +41:12:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.538 195067450260194176 079.38352852263 +41.20857392763 12.3314 11.4767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195986_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 195986_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:49:21.27 +49:49:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.851 991039686095284736 102.33934863711 +49.81704889271 12.6502 12.1511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195992_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 195992_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196001_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196001_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:35.54 +41:04:06.1: 11.69 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:35.54 +41:04:06.1: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
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Considering the candidate 196004_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196004_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:16.61 +41:32:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.644 195079132571769088 079.56899251002 +41.53963219469 12.1662 11.1594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196005_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196005_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:04.19 +41:31:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 1.524 195089341713174144 079.51770745618 +41.52149104768 12.3980 11.9402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196009_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196009_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196017_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196017_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:15:03.60 +48:49:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.264 969337323724612608 093.76493977175 +48.82277166858 12.8238 12.2993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196020_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196020_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196026_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196026_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196027_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196027_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:56.60 +41:57:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196032_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196032_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:49:13.95 +49:47:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.494 991019143267756672 102.30854452623 +49.79817572656 12.7497 12.0783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196040_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196040_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196044_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196044_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196047_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196047_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:43.57 +41:39:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.779 195103734144435712 079.68135550243 +41.66077683365 12.1531 10.9881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196051_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196051_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196057_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196057_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196058_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196058_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196063_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196063_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196064_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196064_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:59.20 +40:58:46.2: 11.87 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:59.20 +40:58:46.2: 12.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.02
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Considering the candidate 196072_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196072_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:34.69 +42:05:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 2.066 195163210851532544 079.39457599153 +42.08781543970 12.4926 11.9842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196073_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196073_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:01.77 +41:55:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 3.085 195161114907497472 079.25827546045 +41.92477108512 12.3945 12.0599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196075_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196075_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:49.06 +44:36:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196078_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196078_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:00.84 +40:56:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 2.913 194837892855047168 080.25408982422 +40.93988008948 12.3796 11.4245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196079_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196079_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:57.63 +40:55:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 2.678 188868369343257984 079.49008802443 +40.91858983115 12.2647 11.2620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196083_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196083_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196089_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196089_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:20.53 +40:53:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 2.619 189055015742029696 079.33599479066 +40.88363609678 12.5721 12.2731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196096_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196096_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196097_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196097_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196098_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196098_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:13:46.68 +44:43:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.408 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196100_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196100_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:13.51 +42:15:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 1.467 195192176110973568 079.55616664542 +42.25649192203 12.3806 11.3692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196101_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196101_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196107_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196107_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196108_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196108_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196127_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196127_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196129_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196129_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:22.73 +42:04:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.688 195166097069555584 079.34479145676 +42.08111693927 12.5159 11.6794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196130_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196130_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:13.43 +42:15:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.136 207178330322063616 079.30601738625 +42.25132498094 12.5273 11.6920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196132_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196132_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:21:47.23 +40:58:16.7: 11.80 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:21:47.23 +40:58:16.7: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
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Considering the candidate 196133_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196133_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196134_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196134_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196136_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196136_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:18.34 +42:06:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.690 195166444965450752 079.32646287745 +42.11230971756 12.5880 11.7826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196140_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196140_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:08:19.80 +41:02:07.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196146_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196146_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196147_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196147_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:53.79 +41:40:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 3.363 195095384728581376 079.47289498649 +41.67794157851 11.7210 10.3108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196149_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196149_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:11.89 +41:36:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.668 195094319576125184 079.29978926721 +41.60696141845 12.5906 12.1561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196153_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196153_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196155_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196155_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196157_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196157_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196160_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196160_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:23.47 +48:55:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196167_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196167_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:30.39 +40:58:14.7: 11.73 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:30.39 +40:58:14.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
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Considering the candidate 196168_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196168_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196170_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196170_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196173_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196173_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:57.57 +40:53:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 1.735 194859028386544256 079.74030146604 +40.89578052582 12.5753 12.1376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196176_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196176_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:22:39.72 +47:54:48.4: 11.89 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:39.72 +47:54:48.4: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
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Considering the candidate 196179_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196179_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196180_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196180_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196181_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196181_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196182_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196182_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196183_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196183_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:55:43.80 +41:06:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196187_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196187_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196188_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196188_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:56.36 +41:52:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 2.662 195147783329012736 079.23516230074 +41.87683013860 12.6007 12.0401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196192_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196192_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196194_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196194_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196195_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196195_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196196_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196196_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196199_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196199_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:51.08 +41:27:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.454 195074910623305344 079.71319319097 +41.45318964569 12.6543 12.4609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196200_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196200_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:32:51.86 +42:57:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196201_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196201_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:23.70 +41:19:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.065 194896716722619520 080.34911335712 +41.33157984265 12.7153 12.0746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196205_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196205_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:56.48 +41:04:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196207_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196207_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196209_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196209_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:47.16 +41:21:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 1.093 194905826350034688 079.94681393071 +41.35475302182 12.6437 11.8765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196216_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196216_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:59.46 +41:39:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 1.216 195106345486579200 079.99817373017 +41.66317352732 12.6349 12.3875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196223_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196223_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:23:32.96 +40:55:48.8: 11.93 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:23:32.96 +40:55:48.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
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Considering the candidate 196227_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196227_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196231_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196231_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196233_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196233_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196235_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196235_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196239_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196239_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196245_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196245_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:57.70 +40:59:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 2.197 194871466611809920 079.74037097414 +40.99016837400 12.4281 11.5540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196253_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196253_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:24:46.97 +41:42:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196256_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196256_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:11.94 +41:32:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.661 194903176353430016 080.29997020346 +41.53680328537 12.6053 11.6877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196260_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196260_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:05:50.20 +44:39:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.688 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196261_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196261_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:40.59 +41:56:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.693 195207401774469376 080.16886920849 +41.94552560749 12.6675 11.6611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196262_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196262_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:02.55 +41:33:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.245 195098962439822208 079.76085503835 +41.55368873254 12.7319 12.0561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196265_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196265_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:24.00 +42:06:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.390 195166273166758272 079.35019614962 +42.10129676461 12.5777 11.7849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196274_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196274_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196275_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196275_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196276_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196276_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196277_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196277_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:38.11 +41:33:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.549 195093494942406016 079.40873547109 +41.56528932958 12.5243 11.6693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196282_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196282_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196286_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196286_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:40:51.33 +48:19:21.6: 12.18 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:40:51.33 +48:19:21.6: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
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Considering the candidate 196289_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196289_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196290_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196290_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:54.82 +41:03:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.786 194866548871392384 079.97888632469 +41.05954152004 12.7000 12.0059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196291_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:34.00 +41:10:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 1.464 194888371603320064 080.14187404385 +41.17937446513 12.6161 11.7005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196292_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196292_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196299_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196299_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:45.05 +41:32:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.445 194913660370288384 080.18787138376 +41.53543706399 12.6224 11.7420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196302_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196302_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:12.76 +40:56:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 2.384 194823534776991360 080.55357188750 +40.94824594931 12.7185 12.2454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196304_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196304_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196305_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196305_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196308_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196308_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:44.75 +46:30:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196311_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196311_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196317_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196317_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196324_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196324_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:57:08.53 +49:03:09.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196325_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196325_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:23:06.97 +40:55:40.8: 12.17 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:23:06.97 +40:55:40.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
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Considering the candidate 196327_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196327_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:59.16 +41:08:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 1.063 194843974524215936 080.49671677564 +41.14069046518 12.7872 12.2632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196332_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196332_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196336_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196336_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196337_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196337_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196339_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196339_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:40:26.06 +48:47:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196344_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196344_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196346_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196346_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196349_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196349_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:24.17 +41:38:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 0.875 195094667472618240 079.35091675898 +41.64251986314 12.8711 12.5147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196352_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196352_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196354_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196354_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:21.86 +42:09:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.349 195187606265772160 079.59173152393 +42.15303664736 12.8344 12.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196355_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196355_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:56:55.54 +45:30:19.2: 8.81 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:56:55.54 +45:30:19.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 8.90 +/- 0.00
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Considering the candidate 196357_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196357_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:06.58 +42:07:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.976 195186270534819712 079.52741258271 +42.11900670668 12.7823 11.9529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196359_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196359_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:57:46.05 +45:53:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.150 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196361_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196361_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:24:40.72 +44:01:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.686 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196362_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196362_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196364_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196364_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196371_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196371_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:19:45.45 +41:21:35.6: 12.11 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:19:45.45 +41:21:35.6: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
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Considering the candidate 196374_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196374_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:04.87 +41:54:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 2.542 195149363876976000 079.27037110900 +41.91082403744 12.8173 12.0008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196378_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196378_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196381_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196381_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196382_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196382_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196385_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196385_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196388_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196388_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196390_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196390_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196393_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196393_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:27.81 +41:10:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 0.182 194880022186588160 079.86581223003 +41.17478774766 12.8919 11.9618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196395_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196395_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:02.39 +41:14:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.399 194882904107286912 079.76001361043 +41.24522468472 12.8266 11.8985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196396_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196396_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196403_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196403_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196406_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196406_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:04.80 +41:13:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.351 194882801027298560 079.76991696732 +41.22373077142 12.8958 12.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196407_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196407_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196412_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196412_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:16.05 +41:34:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 2.060 195099439179168512 079.81755347889 +41.57840311369 12.8022 12.3077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196417_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196417_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196423_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196423_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:23.18 +40:57:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.994 194829165476984064 080.59692104137 +40.95587506780 12.9161 12.1815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196428_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196428_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196438_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196438_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:07.38 +41:49:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 1.750 195120673496413568 079.53053292986 +41.82784725324 12.3862 11.3125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196441_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196441_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:17.75 +41:22:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.252 194906440529323264 080.07430654975 +41.37331302853 12.9911 12.4893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196443_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196443_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:43.76 +41:27:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.006 195075151141475712 079.68213569864 +41.46115359586 12.7378 11.8482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196444_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196444_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:45.03 +41:04:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.697 194886408800174848 080.18756953742 +41.07028059155 13.0982 12.2288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196448_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196448_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:53:12.02 +45:24:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.688 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196450_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196450_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:00.71 +41:30:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.274 195089303054326656 079.50338354099 +41.50715422567 13.0078 12.5486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196451_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196451_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:28:43.72 +41:18:08.6: 11.91 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:28:43.72 +41:18:08.6: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
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Considering the candidate 196458_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196458_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:47:58.47 +50:54:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196462_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196462_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196468_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196468_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196469_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196469_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:17:28.76 +45:52:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.159 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196471_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196471_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:13:42.32 +45:31:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196476_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196476_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:40.35 +41:07:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.699 194887130355606400 080.16822796566 +41.12220103806 12.7171 11.6502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196477_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196477_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:39.07 +41:48:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.548 195118547490607104 079.66326886414 +41.80551920068 12.8866 12.4321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196478_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196478_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196479_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196479_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:11.50 +41:00:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 2.251 194830264988610560 080.54829231200 +41.01005376028 12.8236 11.9413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196480_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196480_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196481_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196481_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196484_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196484_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:18.14 +41:13:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.914 194892288613130880 080.07578737013 +41.22318677161 12.7696 11.7574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196490_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196490_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196491_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196491_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196493_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196493_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196494_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196494_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196495_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196495_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:51.48 +42:30:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.292 207199843818147840 079.21473092291 +42.51512927834 12.8135 12.0657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196497_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196497_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:59.57 +41:32:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.173 195087898604248960 079.24854681600 +41.53799217897 13.0409 12.7200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196500_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196500_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196504_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196504_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:20.82 +40:56:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.183 194858680491308672 079.83731285421 +40.93364140766 12.9281 12.5015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196507_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196507_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196512_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196512_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196516_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196516_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:58.84 +41:26:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.230 194910464914681472 079.99499642791 +41.44140033182 12.6728 11.5968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196524_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196524_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196528_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196528_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:39.64 +41:23:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.882 195074322208400768 079.66531986542 +41.39461701705 12.8919 11.9871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196529_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196529_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:12:10.14 +50:14:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196534_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196534_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:23.53 +41:14:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.333 194881259137151872 079.84880616334 +41.25017037599 12.9742 12.6754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196537_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196537_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:41.47 +41:15:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.792 194893044527344000 080.17288380358 +41.25967366223 12.9430 12.2176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196540_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196540_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196541_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196541_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:46:54.28 +49:34:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.055 990931594654341760 101.72573409967 +49.58002629967 13.1964 12.5008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196542_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196542_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196552_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196552_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:24:11.07 +43:58:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196556_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196556_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:08.30 +41:23:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.362 194907166379805056 080.03451011419 +41.38569359364 12.5608 11.3614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196559_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196559_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196562_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196562_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:47:16.17 +46:04:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.919 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196563_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196563_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196572_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196572_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:26.92 +41:15:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.980 195068309253657344 079.36281571674 +41.25852369828 12.8290 12.2601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196581_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196581_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:15:16.34 +50:12:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.053 970929760158470016 093.81837755340 +50.21676049280 13.4401 12.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196584_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196584_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:18.48 +41:23:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.335 194909601625747456 079.82736380707 +41.38752658150 13.1459 12.7500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196589_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196589_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:59:52.68 +44:00:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.459 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196594_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196594_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:41.23 +42:13:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.403 195191214038299520 079.42226714995 +42.22947156279 13.1070 12.7236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196595_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196595_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196598_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196598_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196609_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196609_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196615_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196615_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:22.01 +41:20:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.854 195072505441640064 079.59181025694 +41.34114819765 13.0351 12.1677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196617_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196617_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196627_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196627_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:11:01.08 +47:29:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.306 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196631_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196631_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196635_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196635_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196640_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196640_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:42.70 +40:59:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.024 189057317844474112 079.42814949730 +40.99713752428 12.9987 12.4897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196641_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196641_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:16.53 +41:18:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.307 195072368002693120 079.56920778638 +41.31048553708 13.1620 12.6833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196643_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196643_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:45:59.91 +41:14:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.624 192676360365419264 086.49878011806 +41.24863519669 13.0621 12.1850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196648_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196648_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196658_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196658_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:30:09.12 +46:12:56.2: 11.19 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:30:09.12 +46:12:56.2: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
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Considering the candidate 196659_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196659_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:18.51 +41:23:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.638 194897163399217408 080.32629642714 +41.38930461602 12.7483 11.5537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196660_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196660_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:11:49.29 +45:03:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196664_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196664_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:52:03.73 +49:32:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196667_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196667_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196679_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196679_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:19.35 +41:09:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.491 194879231912618624 079.83093839840 +41.15132615977 13.1511 12.5050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196685_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196685_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196688_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196688_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:47:34.31 +49:38:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.038 991022544881917440 101.89251740483 +49.63951297865 13.3999 12.9264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196691_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196691_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:56:30.86 +46:14:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.812 197751809117411712 089.12908358575 +46.24714326154 13.6175 12.8385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196696_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196696_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:33.10 +41:26:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.142 194898782603561472 080.38792254180 +41.43592820972 13.1299 12.5095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196699_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196699_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196700_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196700_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:24.99 +42:01:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.689 195162046919379200 079.35352134085 +42.02052646270 12.8727 11.7220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196701_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196701_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:54.87 +41:32:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.219 195101779938388352 079.72904838312 +41.53421386678 13.2969 12.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196703_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196703_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196705_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196705_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:23.52 +42:13:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.687 195189019313809024 079.59774580320 +42.22576543808 12.9576 11.9922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196707_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196707_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:18.03 +41:13:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.879 195065392975814528 079.57551444089 +41.23195685054 13.2785 12.8776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196708_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196708_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:22.16 +40:57:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.374 194870641978119040 079.59247072283 +40.96348528985 12.8837 11.8066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196715_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196715_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:17:34.80 +46:23:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196718_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196718_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:22.94 +42:15:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.717 195192107393536000 079.59584445573 +42.26610398778 13.0930 12.2238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196736_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196736_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:01:04.66 +50:00:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196740_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196740_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196741_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196741_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:54.49 +41:58:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 2.934 195160809968378240 079.22741922808 +41.96859601742 13.0673 12.2885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196748_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196748_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196761_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196761_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196762_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196762_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196763_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196763_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196766_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196766_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:05.88 +42:01:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.293 195176508072970752 079.77455404400 +42.01986530854 13.2201 12.8594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196768_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196768_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:25:21.44 +41:56:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196769_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196769_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:25.66 +42:11:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.087 195167677619167232 079.35689616623 +42.19475385534 13.0442 12.2848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196777_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196777_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196778_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196778_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:21.45 +41:47:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.707 195119921880173696 079.58970365366 +41.78935030952 13.0604 12.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196780_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196780_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196781_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196781_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:33.44 +40:57:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.370 194836003063356288 080.38981245693 +40.96199279485 12.9483 12.4768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196788_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196788_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:18.55 +41:14:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.424 194846173547469824 080.57772852689 +41.23719888363 13.0863 12.6819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196790_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196790_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196798_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:18.42 +41:31:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.038 194903283729274240 080.32705381582 +41.52265636229 13.1447 12.5167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196800_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196800_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:40:14.20 +50:00:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196801_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196801_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:41.28 +41:16:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.277 195071509009355520 079.67194800672 +41.26954478413 12.9224 12.1318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196804_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196804_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196805_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196805_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:08.09 +41:36:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.336 195102428476406272 079.78339517055 +41.60823227311 13.0231 12.0761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196809_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196809_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:44:48.18 +48:58:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196841_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196841_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:43.89 +41:43:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.518 195107651156869376 079.93306736683 +41.73067562732 13.2301 12.5869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196842_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196842_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:47:45.26 +50:03:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.452 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196846_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196846_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196850_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196850_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196856_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196856_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:36.17 +41:35:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.036 195093598021619712 079.40105171147 +41.59909259249 13.1777 12.2651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196869_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196869_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196872_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196872_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:15:42.89 +42:02:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196877_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196877_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196880_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196880_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:00:14.00 +47:43:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.110 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196885_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196885_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:42.84 +41:06:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.100 194887169012493440 080.17896529532 +41.11472822087 12.9603 11.9387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196887_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196887_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196895_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196895_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:22:17.49 +41:20:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.247 194943686483593472 080.57324597254 +41.34609481436 13.3470 12.6544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196901_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196901_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:24:06.06 +40:56:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.357 194166675360205440 081.02512045790 +40.93392919978 13.1038 12.1971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196906_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196906_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:12.82 +42:07:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.424 195178019901628288 079.80325791939 +42.13086103143 13.4280 12.8927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196907_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196907_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:06.55 +41:45:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.339 195107208776848640 080.02740886305 +41.75454825410 13.1414 12.4986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196926_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196926_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:24.27 +41:14:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.534 194895174831417600 080.35154258584 +41.24642694397 13.1908 12.4919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196929_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196929_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:42.18 +41:16:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.062 194881460999313280 079.92722115146 +41.27016445230 13.3005 12.8918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196936_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196936_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:49:13.88 +49:25:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.444 991004712177679232 102.30881205068 +49.42629135664 13.7564 13.2759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196942_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196942_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196945_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196945_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:01:40.39 +44:57:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.605 963004957085784576 090.41950077889 +44.96363164350 13.6794 13.1731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196961_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196961_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196962_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196962_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:48:00.59 +49:23:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.510 990912795581327360 102.00264537972 +49.39281617506 13.6929 13.0146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196967_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 196967_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:16:49.95 +42:02:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.766 195164280301948288 079.20764873705 +42.03337672041 13.0164 12.0131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196977_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196977_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 196986_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 196986_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 197003_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 197003_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:15:49.43 +47:42:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.212 968813234635537152 093.95590182109 +47.71357261547 13.8786 13.1179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197013_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 197013_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:48:17.45 +48:53:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.086 990873217459014656 102.07230191075 +48.89255667340 13.8467 13.3910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197014_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 197014_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:20.16 +41:12:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.218 194881018618999296 079.83449000620 +41.20292316786 13.1752 12.3782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197020_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 197020_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:46.26 +41:37:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.168 195100542988097920 079.94317793840 +41.62860902957 13.2646 12.2226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197026_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 197026_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:17:56.23 +41:46:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.550 195120501697599616 079.48481966236 +41.78284097143 13.2629 12.8360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197044_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 197044_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 128047_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 128047_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:59:44.06 +47:37:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123829_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 123829_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:14:59.10 +46:47:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181970_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 181970_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:21:23.53 +40:58:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.907 194835315869223808 080.34855281787 +40.96999811447 12.7309 12.1502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 126611_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 126611_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 156828_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 156828_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:37:56.86 +44:40:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186923_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 186923_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 169071_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 169071_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167168_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 167168_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:57:23.94 +48:22:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124566_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 124566_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 132003_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 132003_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:48.42 +42:28:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 2.184 207210697198555520 079.70194739375 +42.47874428242 11.6807 10.6117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 123035_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 123035_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 184975_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 184975_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:24:24.23 +41:09:03.9: 12.56 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:24:24.23 +41:09:03.9: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
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Considering the candidate 121731_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 121731_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 111171_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 111171_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 162764_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 162764_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 121947_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 121947_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 155365_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 155365_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:49.24 +40:57:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:27:04.74 +50:07:22.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 183262_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 183262_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 157570_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 157570_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 167810_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 167810_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 169188_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 169188_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:21.36 +41:53:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182669_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 182669_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:19:49.67 +41:39:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.645 195106482925532800 079.95701232771 +41.66056345993 12.7661 12.0970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182099_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 182099_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:23.46 +40:55:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.975 194869984845664384 079.59824037649 +40.92853981800 12.5734 12.0561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148393_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 148393_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:18:28.48 +43:23:12.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 181590_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 181590_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 05:20:18.78 +41:18:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169780_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 169780_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 08610_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 08610_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:45:45.32 +49:42:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170052_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 170052_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 162175_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 162175_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020 did not pass the final checks
**** FOUND 06:26:01.75 +50:29:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161118_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 161118_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 170358_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 170358_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 125643_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 125643_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 140017_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 140017_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
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Considering the candidate 144551_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
Preparing report for the candidate 144551_fd_Aur-02-Q1b1x1_2026-04-22_23-34-16_20.00sec_-4.90C_LIGHTs_0020
make_report_in_HTML.sh Phase 2 (HTML assembly): 20s
make_report_in_HTML.sh TOTAL: 546s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:27:04.73 +50:07:23.2
05:18:28.49 +43:23:12.9
05:17:17.06 +44:00:18.5
05:18:08.85 +41:26:54.6
05:20:07.62 +41:33:55.9
05:17:41.16 +41:50:36.2
05:22:46.02 +42:02:53.9
05:22:15.12 +42:05:43.5
05:18:33.75 +42:05:19.0
05:18:25.61 +42:09:12.0
05:20:26.35 +42:15:37.0
05:18:31.68 +42:55:08.6
05:17:01.77 +43:09:35.5
05:25:13.31 +41:05:11.4
05:20:55.85 +41:05:48.5
05:24:56.28 +41:22:19.1
05:19:10.19 +41:22:36.5
05:17:57.56 +41:23:11.9
05:20:52.03 +41:45:37.0
05:19:36.86 +41:50:09.1
05:17:39.42 +41:49:36.5
05:21:07.49 +41:56:40.4
05:18:06.86 +41:54:42.3
05:23:17.15 +42:01:32.0
05:17:46.24 +41:44:25.9
05:22:21.30 +41:29:28.5
06:24:03.79 +44:40:33.8
05:18:04.61 +44:13:03.0
05:20:12.06 +41:50:45.1
05:22:38.68 +42:27:33.6
06:16:43.96 +44:42:40.5
05:20:53.49 +43:20:16.7
06:08:41.39 +41:19:36.9
05:16:32.32 +43:44:08.9
05:18:33.91 +42:17:09.8
05:24:34.69 +41:13:46.4
05:20:41.08 +43:25:39.7
05:24:31.04 +42:18:55.1
05:19:36.85 +42:36:22.3
05:18:30.28 +43:23:29.8
05:18:09.68 +42:30:21.8
05:17:21.25 +43:43:46.9
05:16:52.88 +42:07:31.6
05:17:50.18 +41:52:05.9
05:19:47.63 +40:57:28.0
05:21:11.83 +40:58:15.5
05:19:37.57 +41:21:38.6
05:17:56.22 +41:11:56.5
05:18:09.76 +40:56:38.3
05:17:58.67 +41:54:50.1
05:17:04.59 +41:49:58.0
05:19:09.52 +41:39:36.5
05:20:34.14 +41:32:12.4
05:19:17.13 +41:01:57.9
05:17:43.68 +41:05:44.2
05:20:36.24 +41:26:10.9
05:19:59.12 +40:55:10.5
05:17:27.03 +42:04:46.0
05:21:26.78 +41:09:41.1
05:21:19.27 +40:58:22.2
05:19:32.68 +41:34:44.4
05:19:44.90 +41:25:28.8
05:19:31.24 +41:15:46.4
05:20:09.95 +41:28:55.1
05:19:26.45 +41:33:40.0
05:17:39.16 +41:50:01.0
05:18:00.23 +41:05:42.0
05:19:51.14 +40:54:04.5
05:17:57.77 +41:10:44.5
05:18:13.00 +41:37:19.8
05:21:47.64 +41:19:19.6
05:19:09.37 +41:40:20.0
05:18:09.11 +42:18:27.1
05:21:28.74 +41:03:43.8
05:17:01.76 +41:52:11.1
05:21:16.64 +41:18:05.5
05:17:38.02 +41:40:02.0
05:21:03.45 +40:57:03.1
05:20:57.31 +41:19:28.7
05:19:30.54 +41:29:14.0
05:17:22.75 +42:24:38.3
05:20:27.78 +41:00:57.8
05:20:09.00 +41:38:29.3
05:18:35.38 +41:27:42.3
05:17:08.60 +41:43:48.8
05:19:34.02 +41:42:04.8
05:18:11.73 +41:06:05.5
05:20:37.17 +41:03:53.1
05:19:41.69 +41:41:45.5
05:17:44.62 +41:41:19.9
05:17:14.40 +41:46:08.7
05:18:07.11 +41:46:17.0
05:17:40.00 +41:57:06.9
05:18:13.74 +41:50:13.8
05:17:50.58 +40:59:14.2
05:17:15.88 +42:10:20.7
05:17:02.25 +41:48:42.7
05:17:07.88 +42:00:29.7
05:17:43.48 +41:35:28.2
05:21:53.86 +41:14:46.1
05:20:59.01 +40:58:25.8
05:17:29.03 +41:47:23.6
05:19:01.33 +41:46:25.8
05:17:15.30 +42:00:41.2
05:19:34.56 +41:44:04.0
05:17:03.28 +41:28:02.5
05:19:22.67 +41:06:10.6
05:17:41.78 +41:24:12.1
05:19:09.42 +41:18:59.1
05:18:03.55 +42:06:18.5
05:17:18.76 +42:27:03.9
05:19:40.99 +41:28:15.9
05:17:45.72 +41:41:57.8
05:18:24.57 +41:48:04.5
05:17:41.79 +41:03:14.7
05:18:25.87 +42:08:49.6
05:18:09.63 +42:06:05.5
05:18:19.13 +41:00:06.2
05:17:22.15 +41:40:33.6
05:20:13.91 +41:33:22.4
05:17:15.84 +41:12:38.4
05:18:36.21 +41:46:23.8
05:18:13.52 +41:41:03.5
05:17:59.36 +42:12:01.2
05:17:58.28 +41:41:03.5
05:18:59.13 +41:42:18.2
05:21:56.13 +41:24:48.4
05:19:56.49 +41:31:31.5
05:19:45.11 +41:19:52.9
05:17:23.79 +40:56:49.1
05:17:57.69 +41:51:47.5
05:17:22.79 +41:57:52.3
05:18:09.87 +41:34:39.5
05:19:19.10 +41:59:23.2
05:17:20.63 +41:54:56.5
05:19:30.19 +41:56:21.0
05:17:51.67 +41:13:13.5
05:17:23.36 +42:32:04.8
05:17:31.56 +42:08:57.1
05:18:56.89 +41:23:06.9
05:17:41.86 +41:12:31.6
05:22:02.87 +40:59:16.6
05:19:23.07 +41:17:39.0
05:17:22.21 +41:36:53.2
05:17:15.02 +41:43:32.7
05:17:13.09 +41:44:46.8
05:17:22.91 +41:57:26.6
05:21:27.30 +41:18:34.6
05:17:16.80 +41:55:39.1
05:18:33.43 +41:04:56.1
05:18:34.48 +41:19:31.6
05:18:42.48 +41:33:09.0
05:31:45.51 +51:02:32.1
05:22:15.07 +41:08:09.0
05:19:36.72 +41:02:30.2
05:17:25.80 +41:01:31.9
05:17:43.47 +41:02:37.1
06:09:33.54 +43:09:03.8
05:17:49.92 +41:19:53.8
05:17:36.05 +41:41:02.4
05:17:42.33 +42:09:26.8
05:17:29.48 +41:17:17.1
05:16:57.48 +42:27:00.6
05:19:53.85 +41:09:16.5
05:19:19.62 +40:59:12.5
05:21:07.55 +41:01:50.2
05:17:46.25 +41:26:53.2
05:17:32.96 +42:23:23.0
05:18:52.23 +41:48:27.7
05:21:11.00 +41:07:23.0
05:21:43.91 +40:55:58.4
05:33:40.19 +48:17:45.2
05:22:26.82 +41:02:54.2
05:18:13.49 +41:50:58.2
05:18:22.38 +41:29:29.8
05:19:39.30 +41:16:19.8
05:20:34.35 +41:18:00.6
05:19:33.37 +41:30:24.1
05:17:22.06 +41:29:30.2
05:18:01.96 +41:23:18.1
05:18:21.62 +41:34:57.8
05:21:46.28 +41:06:10.3
05:18:11.62 +41:27:00.6
05:19:01.04 +41:43:45.8
05:17:44.50 +42:11:19.3
05:21:35.86 +41:17:58.9
05:17:43.54 +41:23:54.6
06:11:06.00 +41:55:49.6
05:18:45.14 +42:03:00.3
05:21:04.81 +41:33:48.6
05:21:17.63 +41:12:01.4
05:17:28.80 +41:49:34.7
05:17:04.64 +42:26:01.3
05:20:28.44 +41:37:05.0
05:20:28.88 +41:41:24.3
06:26:19.97 +41:59:11.2
05:21:01.13 +41:24:15.2
05:17:48.68 +41:41:34.0
05:21:46.41 +41:09:51.6
05:18:23.67 +41:28:28.5
05:21:03.53 +41:02:20.3
05:18:38.13 +42:14:06.1
05:19:43.62 +41:22:52.2
05:21:35.75 +41:24:39.2
05:17:03.54 +42:00:52.5
05:17:59.26 +41:42:14.4
05:19:42.64 +41:26:17.8
05:21:03.21 +41:27:00.1
05:20:32.66 +41:09:01.5
05:20:05.17 +41:14:24.8
05:17:28.53 +41:13:52.7
05:20:29.97 +41:51:22.7
05:19:37.73 +41:47:12.4
06:48:33.97 +49:51:14.5
06:24:51.95 +43:32:25.8
05:20:42.92 +40:54:42.0
05:47:15.81 +43:29:09.2
05:17:52.95 +41:57:10.7
06:16:36.27 +44:32:55.4
05:17:18.71 +42:19:03.8
05:40:43.00 +48:20:10.6
05:17:33.46 +41:45:08.1
05:21:48.20 +41:07:18.4
05:19:05.62 +41:12:55.9
05:17:09.43 +41:50:12.7
05:43:53.04 +47:06:14.7
05:17:38.65 +42:14:41.9
05:16:44.56 +42:12:54.0
05:18:15.39 +41:28:35.9
05:20:46.01 +40:57:08.7
05:22:00.78 +41:12:01.9
05:19:31.37 +41:08:13.6
05:40:17.56 +46:01:05.4
05:22:12.40 +41:06:52.8
05:20:04.97 +41:39:14.0
05:22:56.32 +40:57:00.2
05:28:01.16 +48:14:58.9
05:17:44.79 +41:17:54.0
05:20:41.60 +49:23:44.5
05:21:02.28 +40:59:50.8
05:47:22.10 +46:02:51.4
05:20:00.07 +41:39:11.7
05:20:56.82 +41:41:27.6
05:19:18.46 +41:43:23.0
05:18:48.90 +41:33:08.5
05:18:33.51 +40:55:58.4
05:18:19.07 +42:20:17.5
05:21:14.48 +41:05:09.5
05:18:47.20 +41:36:34.4
05:17:16.13 +41:16:54.2
05:17:45.94 +42:13:18.5
05:18:20.57 +41:53:19.0
05:20:34.96 +40:57:01.5
05:18:13.25 +41:29:51.2
06:12:44.60 +47:30:42.7
06:13:33.56 +48:03:18.0
06:01:16.84 +47:35:44.3
06:09:52.02 +46:34:27.5
########### Completed Aur-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:18:28.49 +43:23:12.9
05:27:04.73 +50:07:23.2
06:24:03.79 +44:40:33.8
05:18:04.61 +44:13:03.0
05:20:12.06 +41:50:45.1
05:22:38.68 +42:27:33.6
06:16:43.96 +44:42:40.5
05:20:53.49 +43:20:16.7
06:08:41.39 +41:19:36.9
05:16:32.32 +43:44:08.9
05:18:33.91 +42:17:09.8
05:24:34.69 +41:13:46.4
05:20:41.08 +43:25:39.7
05:24:31.04 +42:18:55.1
05:19:36.85 +42:36:22.3
05:18:30.28 +43:23:29.8
05:18:09.68 +42:30:21.8
05:17:21.25 +43:43:46.9
05:16:52.88 +42:07:31.6
05:17:50.18 +41:52:05.9
05:19:47.63 +40:57:28.0
05:21:11.83 +40:58:15.5
05:19:37.57 +41:21:38.6
05:17:56.22 +41:11:56.5
05:18:09.76 +40:56:38.3
05:17:58.67 +41:54:50.1
05:17:04.59 +41:49:58.0
05:19:09.52 +41:39:36.5
05:20:34.14 +41:32:12.4
05:19:17.13 +41:01:57.9
05:17:43.68 +41:05:44.2
05:20:36.24 +41:26:10.9
05:19:59.12 +40:55:10.5
05:17:27.03 +42:04:46.0
05:21:26.78 +41:09:41.1
05:21:19.27 +40:58:22.2
05:19:32.68 +41:34:44.4
05:19:44.90 +41:25:28.8
05:19:31.24 +41:15:46.4
05:20:09.95 +41:28:55.1
05:19:26.45 +41:33:40.0
05:17:39.16 +41:50:01.0
05:18:00.23 +41:05:42.0
05:19:51.14 +40:54:04.5
05:17:57.77 +41:10:44.5
05:18:13.00 +41:37:19.8
05:21:47.64 +41:19:19.6
05:19:09.37 +41:40:20.0
05:18:09.11 +42:18:27.1
05:21:28.74 +41:03:43.8
05:17:01.76 +41:52:11.1
05:21:16.64 +41:18:05.5
05:17:38.02 +41:40:02.0
05:21:03.45 +40:57:03.1
05:20:57.31 +41:19:28.7
05:19:30.54 +41:29:14.0
05:17:22.75 +42:24:38.3
05:20:27.78 +41:00:57.8
05:20:09.00 +41:38:29.3
05:18:35.38 +41:27:42.3
05:17:08.60 +41:43:48.8
05:19:34.02 +41:42:04.8
05:18:11.73 +41:06:05.5
05:20:37.17 +41:03:53.1
05:19:41.69 +41:41:45.5
05:17:44.62 +41:41:19.9
05:17:14.40 +41:46:08.7
05:18:07.11 +41:46:17.0
05:17:40.00 +41:57:06.9
05:18:13.74 +41:50:13.8
05:17:50.58 +40:59:14.2
05:17:15.88 +42:10:20.7
05:17:02.25 +41:48:42.7
05:17:07.88 +42:00:29.7
05:17:43.48 +41:35:28.2
05:21:53.86 +41:14:46.1
05:20:59.01 +40:58:25.8
05:17:29.03 +41:47:23.6
05:19:01.33 +41:46:25.8
05:17:15.30 +42:00:41.2
05:19:34.56 +41:44:04.0
05:17:03.28 +41:28:02.5
05:19:22.67 +41:06:10.6
05:17:41.78 +41:24:12.1
05:19:09.42 +41:18:59.1
05:18:03.55 +42:06:18.5
05:17:18.76 +42:27:03.9
05:19:40.99 +41:28:15.9
05:17:45.72 +41:41:57.8
05:18:24.57 +41:48:04.5
05:17:41.79 +41:03:14.7
05:18:25.87 +42:08:49.6
05:18:09.63 +42:06:05.5
05:18:19.13 +41:00:06.2
05:17:22.15 +41:40:33.6
05:20:13.91 +41:33:22.4
05:17:15.84 +41:12:38.4
05:18:36.21 +41:46:23.8
05:18:13.52 +41:41:03.5
05:17:59.36 +42:12:01.2
05:17:58.28 +41:41:03.5
05:18:59.13 +41:42:18.2
05:21:56.13 +41:24:48.4
05:19:56.49 +41:31:31.5
05:19:45.11 +41:19:52.9
05:17:23.79 +40:56:49.1
05:17:57.69 +41:51:47.5
05:17:22.79 +41:57:52.3
05:18:09.87 +41:34:39.5
05:19:19.10 +41:59:23.2
05:17:20.63 +41:54:56.5
05:19:30.19 +41:56:21.0
05:17:51.67 +41:13:13.5
05:17:23.36 +42:32:04.8
05:17:31.56 +42:08:57.1
05:18:56.89 +41:23:06.9
05:17:41.86 +41:12:31.6
05:22:02.87 +40:59:16.6
05:19:23.07 +41:17:39.0
05:17:22.21 +41:36:53.2
05:17:15.02 +41:43:32.7
05:17:13.09 +41:44:46.8
05:17:22.91 +41:57:26.6
05:21:27.30 +41:18:34.6
05:17:16.80 +41:55:39.1
05:18:33.43 +41:04:56.1
05:18:34.48 +41:19:31.6
05:18:42.48 +41:33:09.0
05:31:45.51 +51:02:32.1
05:22:15.07 +41:08:09.0
05:19:36.72 +41:02:30.2
05:17:25.80 +41:01:31.9
05:17:43.47 +41:02:37.1
06:09:33.54 +43:09:03.8
05:17:49.92 +41:19:53.8
05:17:36.05 +41:41:02.4
05:17:42.33 +42:09:26.8
05:17:29.48 +41:17:17.1
05:16:57.48 +42:27:00.6
05:19:53.85 +41:09:16.5
05:19:19.62 +40:59:12.5
05:21:07.55 +41:01:50.2
05:17:46.25 +41:26:53.2
05:17:32.96 +42:23:23.0
05:18:52.23 +41:48:27.7
05:21:11.00 +41:07:23.0
05:21:43.91 +40:55:58.4
05:33:40.19 +48:17:45.2
05:22:26.82 +41:02:54.2
05:18:13.49 +41:50:58.2
05:18:22.38 +41:29:29.8
05:19:39.30 +41:16:19.8
05:20:34.35 +41:18:00.6
05:19:33.37 +41:30:24.1
05:17:22.06 +41:29:30.2
05:18:01.96 +41:23:18.1
05:18:21.62 +41:34:57.8
05:21:46.28 +41:06:10.3
05:18:11.62 +41:27:00.6
05:19:01.04 +41:43:45.8
05:17:44.50 +42:11:19.3
05:21:35.86 +41:17:58.9
05:17:43.54 +41:23:54.6
06:11:06.00 +41:55:49.6
05:18:45.14 +42:03:00.3
05:21:04.81 +41:33:48.6
05:21:17.63 +41:12:01.4
05:17:28.80 +41:49:34.7
05:17:04.64 +42:26:01.3
05:20:28.44 +41:37:05.0
05:20:28.88 +41:41:24.3
06:26:19.97 +41:59:11.2
05:21:01.13 +41:24:15.2
05:17:48.68 +41:41:34.0
05:21:46.41 +41:09:51.6
05:18:23.67 +41:28:28.5
05:21:03.53 +41:02:20.3
05:18:38.13 +42:14:06.1
05:19:43.62 +41:22:52.2
05:21:35.75 +41:24:39.2
05:17:03.54 +42:00:52.5
05:17:59.26 +41:42:14.4
05:19:42.64 +41:26:17.8
05:21:03.21 +41:27:00.1
05:20:32.66 +41:09:01.5
05:20:05.17 +41:14:24.8
05:17:28.53 +41:13:52.7
05:20:29.97 +41:51:22.7
05:19:37.73 +41:47:12.4
06:48:33.97 +49:51:14.5
06:24:51.95 +43:32:25.8
05:20:42.92 +40:54:42.0
05:47:15.81 +43:29:09.2
05:17:52.95 +41:57:10.7
06:16:36.27 +44:32:55.4
05:17:18.71 +42:19:03.8
05:40:43.00 +48:20:10.6
05:17:33.46 +41:45:08.1
05:21:48.20 +41:07:18.4
05:19:05.62 +41:12:55.9
05:17:09.43 +41:50:12.7
05:43:53.04 +47:06:14.7
05:17:38.65 +42:14:41.9
05:16:44.56 +42:12:54.0
05:18:15.39 +41:28:35.9
05:20:46.01 +40:57:08.7
05:22:00.78 +41:12:01.9
05:19:31.37 +41:08:13.6
05:40:17.56 +46:01:05.4
05:22:12.40 +41:06:52.8
05:20:04.97 +41:39:14.0
05:22:56.32 +40:57:00.2
05:28:01.16 +48:14:58.9
05:17:44.79 +41:17:54.0
05:20:41.60 +49:23:44.5
05:21:02.28 +40:59:50.8
05:47:22.10 +46:02:51.4
05:20:00.07 +41:39:11.7
05:20:56.82 +41:41:27.6
05:19:18.46 +41:43:23.0
05:18:48.90 +41:33:08.5
05:18:33.51 +40:55:58.4
05:18:19.07 +42:20:17.5
05:21:14.48 +41:05:09.5
05:18:47.20 +41:36:34.4
05:17:16.13 +41:16:54.2
05:17:45.94 +42:13:18.5
05:18:20.57 +41:53:19.0
05:20:34.96 +40:57:01.5
05:18:13.25 +41:29:51.2
06:12:44.60 +47:30:42.7
06:13:33.56 +48:03:18.0
06:01:16.84 +47:35:44.3
05:20:26.35 +42:15:37.0
05:22:46.02 +42:02:53.9
05:18:25.61 +42:09:12.0
05:25:13.31 +41:05:11.4
05:22:21.30 +41:29:28.5
05:17:39.42 +41:49:36.5
05:20:52.03 +41:45:37.0
05:22:15.12 +42:05:43.5
05:17:41.16 +41:50:36.2
05:18:08.85 +41:26:54.6
06:09:52.02 +46:34:27.5
05:17:17.06 +44:00:18.5
05:17:57.56 +41:23:11.9
05:20:07.62 +41:33:55.9
05:17:46.24 +41:44:25.9
05:20:55.85 +41:05:48.5
05:19:36.86 +41:50:09.1
05:21:07.49 +41:56:40.4
05:18:06.86 +41:54:42.3
05:19:10.19 +41:22:36.5
05:24:56.28 +41:22:19.1
05:23:17.15 +42:01:32.0
05:18:33.75 +42:05:19.0
05:18:31.68 +42:55:08.6
05:17:01.77 +43:09:35.5
###################################################################################
05:18:28.49 +43:23:12.9 -- not an asteroid (will add it to exclusion list)
05:27:04.73 +50:07:23.2 -- not an asteroid (will add it to exclusion list)
06:24:03.79 +44:40:33.8 -- not an asteroid (will add it to exclusion list)
05:18:04.61 +44:13:03.0 -- not an asteroid (will add it to exclusion list)
05:20:12.06 +41:50:45.1 -- not an asteroid (will add it to exclusion list)
05:22:38.68 +42:27:33.6 -- not an asteroid (will add it to exclusion list)
06:16:43.96 +44:42:40.5 -- not an asteroid (will add it to exclusion list)
05:20:53.49 +43:20:16.7 -- not an asteroid (will add it to exclusion list)
06:08:41.39 +41:19:36.9 -- not an asteroid (will add it to exclusion list)
05:16:32.32 +43:44:08.9 -- not an asteroid (will add it to exclusion list)
05:18:33.91 +42:17:09.8 -- not an asteroid (will add it to exclusion list)
05:24:34.69 +41:13:46.4 -- not an asteroid (will add it to exclusion list)
05:20:41.08 +43:25:39.7 -- not an asteroid (will add it to exclusion list)
05:24:31.04 +42:18:55.1 -- not an asteroid (will add it to exclusion list)
05:19:36.85 +42:36:22.3 -- not an asteroid (will add it to exclusion list)
05:18:30.28 +43:23:29.8 -- not an asteroid (will add it to exclusion list)
05:18:09.68 +42:30:21.8 -- not an asteroid (will add it to exclusion list)
05:17:21.25 +43:43:46.9 -- not an asteroid (will add it to exclusion list)
05:16:52.88 +42:07:31.6 -- not an asteroid (will add it to exclusion list)
05:17:50.18 +41:52:05.9 -- not an asteroid (will add it to exclusion list)
05:19:47.63 +40:57:28.0 -- not an asteroid (will add it to exclusion list)
05:21:11.83 +40:58:15.5 -- not an asteroid (will add it to exclusion list)
05:19:37.57 +41:21:38.6 -- not an asteroid (will add it to exclusion list)
05:17:56.22 +41:11:56.5 -- not an asteroid (will add it to exclusion list)
05:18:09.76 +40:56:38.3 -- not an asteroid (will add it to exclusion list)
05:17:58.67 +41:54:50.1 -- not an asteroid (will add it to exclusion list)
05:17:04.59 +41:49:58.0 -- not an asteroid (will add it to exclusion list)
05:19:09.52 +41:39:36.5 -- not an asteroid (will add it to exclusion list)
05:20:34.14 +41:32:12.4 -- not an asteroid (will add it to exclusion list)
05:19:17.13 +41:01:57.9 -- not an asteroid (will add it to exclusion list)
05:17:43.68 +41:05:44.2 -- not an asteroid (will add it to exclusion list)
05:20:36.24 +41:26:10.9 -- not an asteroid (will add it to exclusion list)
05:19:59.12 +40:55:10.5 -- not an asteroid (will add it to exclusion list)
05:17:27.03 +42:04:46.0 -- not an asteroid (will add it to exclusion list)
05:21:26.78 +41:09:41.1 -- not an asteroid (will add it to exclusion list)
05:21:19.27 +40:58:22.2 -- not an asteroid (will add it to exclusion list)
05:19:32.68 +41:34:44.4 -- not an asteroid (will add it to exclusion list)
05:19:44.90 +41:25:28.8 -- not an asteroid (will add it to exclusion list)
05:19:31.24 +41:15:46.4 -- not an asteroid (will add it to exclusion list)
05:20:09.95 +41:28:55.1 -- not an asteroid (will add it to exclusion list)
05:19:26.45 +41:33:40.0 -- not an asteroid (will add it to exclusion list)
05:17:39.16 +41:50:01.0 -- not an asteroid (will add it to exclusion list)
05:18:00.23 +41:05:42.0 -- not an asteroid (will add it to exclusion list)
05:19:51.14 +40:54:04.5 -- not an asteroid (will add it to exclusion list)
05:17:57.77 +41:10:44.5 -- not an asteroid (will add it to exclusion list)
05:18:13.00 +41:37:19.8 -- not an asteroid (will add it to exclusion list)
05:21:47.64 +41:19:19.6 -- not an asteroid (will add it to exclusion list)
05:19:09.37 +41:40:20.0 -- not an asteroid (will add it to exclusion list)
05:18:09.11 +42:18:27.1 -- not an asteroid (will add it to exclusion list)
05:21:28.74 +41:03:43.8 -- not an asteroid (will add it to exclusion list)
05:17:01.76 +41:52:11.1 -- not an asteroid (will add it to exclusion list)
05:21:16.64 +41:18:05.5 -- not an asteroid (will add it to exclusion list)
05:17:38.02 +41:40:02.0 -- not an asteroid (will add it to exclusion list)
05:21:03.45 +40:57:03.1 -- not an asteroid (will add it to exclusion list)
05:20:57.31 +41:19:28.7 -- not an asteroid (will add it to exclusion list)
05:19:30.54 +41:29:14.0 -- not an asteroid (will add it to exclusion list)
05:17:22.75 +42:24:38.3 -- not an asteroid (will add it to exclusion list)
05:20:27.78 +41:00:57.8 -- not an asteroid (will add it to exclusion list)
05:20:09.00 +41:38:29.3 -- not an asteroid (will add it to exclusion list)
05:18:35.38 +41:27:42.3 -- not an asteroid (will add it to exclusion list)
05:17:08.60 +41:43:48.8 -- not an asteroid (will add it to exclusion list)
05:19:34.02 +41:42:04.8 -- not an asteroid (will add it to exclusion list)
05:18:11.73 +41:06:05.5 -- not an asteroid (will add it to exclusion list)
05:20:37.17 +41:03:53.1 -- not an asteroid (will add it to exclusion list)
05:19:41.69 +41:41:45.5 -- not an asteroid (will add it to exclusion list)
05:17:44.62 +41:41:19.9 -- not an asteroid (will add it to exclusion list)
05:17:14.40 +41:46:08.7 -- not an asteroid (will add it to exclusion list)
05:18:07.11 +41:46:17.0 -- not an asteroid (will add it to exclusion list)
05:17:40.00 +41:57:06.9 -- not an asteroid (will add it to exclusion list)
05:18:13.74 +41:50:13.8 -- not an asteroid (will add it to exclusion list)
05:17:50.58 +40:59:14.2 -- not an asteroid (will add it to exclusion list)
05:17:15.88 +42:10:20.7 -- not an asteroid (will add it to exclusion list)
05:17:02.25 +41:48:42.7 -- not an asteroid (will add it to exclusion list)
05:17:07.88 +42:00:29.7 -- not an asteroid (will add it to exclusion list)
05:17:43.48 +41:35:28.2 -- not an asteroid (will add it to exclusion list)
05:21:53.86 +41:14:46.1 -- not an asteroid (will add it to exclusion list)
05:20:59.01 +40:58:25.8 -- not an asteroid (will add it to exclusion list)
05:17:29.03 +41:47:23.6 -- not an asteroid (will add it to exclusion list)
05:19:01.33 +41:46:25.8 -- not an asteroid (will add it to exclusion list)
05:17:15.30 +42:00:41.2 -- not an asteroid (will add it to exclusion list)
05:19:34.56 +41:44:04.0 -- not an asteroid (will add it to exclusion list)
05:17:03.28 +41:28:02.5 -- not an asteroid (will add it to exclusion list)
05:19:22.67 +41:06:10.6 -- not an asteroid (will add it to exclusion list)
05:17:41.78 +41:24:12.1 -- not an asteroid (will add it to exclusion list)
05:19:09.42 +41:18:59.1 -- not an asteroid (will add it to exclusion list)
05:18:03.55 +42:06:18.5 -- not an asteroid (will add it to exclusion list)
05:17:18.76 +42:27:03.9 -- not an asteroid (will add it to exclusion list)
05:19:40.99 +41:28:15.9 -- not an asteroid (will add it to exclusion list)
05:17:45.72 +41:41:57.8 -- not an asteroid (will add it to exclusion list)
05:18:24.57 +41:48:04.5 -- not an asteroid (will add it to exclusion list)
05:17:41.79 +41:03:14.7 -- not an asteroid (will add it to exclusion list)
05:18:25.87 +42:08:49.6 -- not an asteroid (will add it to exclusion list)
05:18:09.63 +42:06:05.5 -- not an asteroid (will add it to exclusion list)
05:18:19.13 +41:00:06.2 -- not an asteroid (will add it to exclusion list)
05:17:22.15 +41:40:33.6 -- not an asteroid (will add it to exclusion list)
05:20:13.91 +41:33:22.4 -- not an asteroid (will add it to exclusion list)
05:17:15.84 +41:12:38.4 -- not an asteroid (will add it to exclusion list)
05:18:36.21 +41:46:23.8 -- not an asteroid (will add it to exclusion list)
05:18:13.52 +41:41:03.5 -- not an asteroid (will add it to exclusion list)
05:17:59.36 +42:12:01.2 -- not an asteroid (will add it to exclusion list)
05:17:58.28 +41:41:03.5 -- not an asteroid (will add it to exclusion list)
05:18:59.13 +41:42:18.2 -- not an asteroid (will add it to exclusion list)
05:21:56.13 +41:24:48.4 -- not an asteroid (will add it to exclusion list)
05:19:56.49 +41:31:31.5 -- not an asteroid (will add it to exclusion list)
05:19:45.11 +41:19:52.9 -- not an asteroid (will add it to exclusion list)
05:17:23.79 +40:56:49.1 -- not an asteroid (will add it to exclusion list)
05:17:57.69 +41:51:47.5 -- not an asteroid (will add it to exclusion list)
05:17:22.79 +41:57:52.3 -- not an asteroid (will add it to exclusion list)
05:18:09.87 +41:34:39.5 -- not an asteroid (will add it to exclusion list)
05:19:19.10 +41:59:23.2 -- not an asteroid (will add it to exclusion list)
05:17:20.63 +41:54:56.5 -- not an asteroid (will add it to exclusion list)
05:19:30.19 +41:56:21.0 -- not an asteroid (will add it to exclusion list)
05:17:51.67 +41:13:13.5 -- not an asteroid (will add it to exclusion list)
05:17:23.36 +42:32:04.8 -- not an asteroid (will add it to exclusion list)
05:17:31.56 +42:08:57.1 -- not an asteroid (will add it to exclusion list)
05:18:56.89 +41:23:06.9 -- not an asteroid (will add it to exclusion list)
05:17:41.86 +41:12:31.6 -- not an asteroid (will add it to exclusion list)
05:22:02.87 +40:59:16.6 -- not an asteroid (will add it to exclusion list)
05:19:23.07 +41:17:39.0 -- not an asteroid (will add it to exclusion list)
05:17:22.21 +41:36:53.2 -- not an asteroid (will add it to exclusion list)
05:17:15.02 +41:43:32.7 -- not an asteroid (will add it to exclusion list)
05:17:13.09 +41:44:46.8 -- not an asteroid (will add it to exclusion list)
05:17:22.91 +41:57:26.6 -- not an asteroid (will add it to exclusion list)
05:21:27.30 +41:18:34.6 -- not an asteroid (will add it to exclusion list)
05:17:16.80 +41:55:39.1 -- not an asteroid (will add it to exclusion list)
05:18:33.43 +41:04:56.1 -- not an asteroid (will add it to exclusion list)
05:18:34.48 +41:19:31.6 -- not an asteroid (will add it to exclusion list)
05:18:42.48 +41:33:09.0 -- not an asteroid (will add it to exclusion list)
05:31:45.51 +51:02:32.1 -- not an asteroid (will add it to exclusion list)
05:22:15.07 +41:08:09.0 -- not an asteroid (will add it to exclusion list)
05:19:36.72 +41:02:30.2 -- not an asteroid (will add it to exclusion list)
05:17:25.80 +41:01:31.9 -- not an asteroid (will add it to exclusion list)
05:17:43.47 +41:02:37.1 -- not an asteroid (will add it to exclusion list)
06:09:33.54 +43:09:03.8 -- not an asteroid (will add it to exclusion list)
05:17:49.92 +41:19:53.8 -- not an asteroid (will add it to exclusion list)
05:17:36.05 +41:41:02.4 -- not an asteroid (will add it to exclusion list)
05:17:42.33 +42:09:26.8 -- not an asteroid (will add it to exclusion list)
05:17:29.48 +41:17:17.1 -- not an asteroid (will add it to exclusion list)
05:16:57.48 +42:27:00.6 -- not an asteroid (will add it to exclusion list)
05:19:53.85 +41:09:16.5 -- not an asteroid (will add it to exclusion list)
05:19:19.62 +40:59:12.5 -- not an asteroid (will add it to exclusion list)
05:21:07.55 +41:01:50.2 -- not an asteroid (will add it to exclusion list)
05:17:46.25 +41:26:53.2 -- not an asteroid (will add it to exclusion list)
05:17:32.96 +42:23:23.0 -- not an asteroid (will add it to exclusion list)
05:18:52.23 +41:48:27.7 -- not an asteroid (will add it to exclusion list)
05:21:11.00 +41:07:23.0 -- not an asteroid (will add it to exclusion list)
05:21:43.91 +40:55:58.4 -- not an asteroid (will add it to exclusion list)
05:33:40.19 +48:17:45.2 -- not an asteroid (will add it to exclusion list)
05:22:26.82 +41:02:54.2 -- not an asteroid (will add it to exclusion list)
05:18:13.49 +41:50:58.2 -- not an asteroid (will add it to exclusion list)
05:18:22.38 +41:29:29.8 -- not an asteroid (will add it to exclusion list)
05:19:39.30 +41:16:19.8 -- not an asteroid (will add it to exclusion list)
05:20:34.35 +41:18:00.6 -- not an asteroid (will add it to exclusion list)
05:19:33.37 +41:30:24.1 -- not an asteroid (will add it to exclusion list)
05:17:22.06 +41:29:30.2 -- not an asteroid (will add it to exclusion list)
05:18:01.96 +41:23:18.1 -- not an asteroid (will add it to exclusion list)
05:18:21.62 +41:34:57.8 -- not an asteroid (will add it to exclusion list)
05:21:46.28 +41:06:10.3 -- not an asteroid (will add it to exclusion list)
05:18:11.62 +41:27:00.6 -- not an asteroid (will add it to exclusion list)
05:19:01.04 +41:43:45.8 -- not an asteroid (will add it to exclusion list)
05:17:44.50 +42:11:19.3 -- not an asteroid (will add it to exclusion list)
05:21:35.86 +41:17:58.9 -- not an asteroid (will add it to exclusion list)
05:17:43.54 +41:23:54.6 -- not an asteroid (will add it to exclusion list)
06:11:06.00 +41:55:49.6 -- not an asteroid (will add it to exclusion list)
05:18:45.14 +42:03:00.3 -- not an asteroid (will add it to exclusion list)
05:21:04.81 +41:33:48.6 -- not an asteroid (will add it to exclusion list)
05:21:17.63 +41:12:01.4 -- not an asteroid (will add it to exclusion list)
05:17:28.80 +41:49:34.7 -- not an asteroid (will add it to exclusion list)
05:17:04.64 +42:26:01.3 -- not an asteroid (will add it to exclusion list)
05:20:28.44 +41:37:05.0 -- not an asteroid (will add it to exclusion list)
05:20:28.88 +41:41:24.3 -- not an asteroid (will add it to exclusion list)
06:26:19.97 +41:59:11.2 -- not an asteroid (will add it to exclusion list)
05:21:01.13 +41:24:15.2 -- not an asteroid (will add it to exclusion list)
05:17:48.68 +41:41:34.0 -- not an asteroid (will add it to exclusion list)
05:21:46.41 +41:09:51.6 -- not an asteroid (will add it to exclusion list)
05:18:23.67 +41:28:28.5 -- not an asteroid (will add it to exclusion list)
05:21:03.53 +41:02:20.3 -- not an asteroid (will add it to exclusion list)
05:18:38.13 +42:14:06.1 -- not an asteroid (will add it to exclusion list)
05:19:43.62 +41:22:52.2 -- not an asteroid (will add it to exclusion list)
05:21:35.75 +41:24:39.2 -- not an asteroid (will add it to exclusion list)
05:17:03.54 +42:00:52.5 -- not an asteroid (will add it to exclusion list)
05:17:59.26 +41:42:14.4 -- not an asteroid (will add it to exclusion list)
05:19:42.64 +41:26:17.8 -- not an asteroid (will add it to exclusion list)
05:21:03.21 +41:27:00.1 -- not an asteroid (will add it to exclusion list)
05:20:32.66 +41:09:01.5 -- not an asteroid (will add it to exclusion list)
05:20:05.17 +41:14:24.8 -- not an asteroid (will add it to exclusion list)
05:17:28.53 +41:13:52.7 -- not an asteroid (will add it to exclusion list)
05:20:29.97 +41:51:22.7 -- not an asteroid (will add it to exclusion list)
05:19:37.73 +41:47:12.4 -- not an asteroid (will add it to exclusion list)
06:48:33.97 +49:51:14.5 -- not an asteroid (will add it to exclusion list)
06:24:51.95 +43:32:25.8 -- not an asteroid (will add it to exclusion list)
05:20:42.92 +40:54:42.0 -- not an asteroid (will add it to exclusion list)
05:47:15.81 +43:29:09.2 -- not an asteroid (will add it to exclusion list)
05:17:52.95 +41:57:10.7 -- not an asteroid (will add it to exclusion list)
06:16:36.27 +44:32:55.4 -- not an asteroid (will add it to exclusion list)
05:17:18.71 +42:19:03.8 -- not an asteroid (will add it to exclusion list)
05:40:43.00 +48:20:10.6 -- not an asteroid (will add it to exclusion list)
05:17:33.46 +41:45:08.1 -- not an asteroid (will add it to exclusion list)
05:21:48.20 +41:07:18.4 -- not an asteroid (will add it to exclusion list)
05:19:05.62 +41:12:55.9 -- not an asteroid (will add it to exclusion list)
05:17:09.43 +41:50:12.7 -- not an asteroid (will add it to exclusion list)
05:43:53.04 +47:06:14.7 -- not an asteroid (will add it to exclusion list)
05:17:38.65 +42:14:41.9 -- not an asteroid (will add it to exclusion list)
05:16:44.56 +42:12:54.0 -- not an asteroid (will add it to exclusion list)
05:18:15.39 +41:28:35.9 -- not an asteroid (will add it to exclusion list)
05:20:46.01 +40:57:08.7 -- not an asteroid (will add it to exclusion list)
05:22:00.78 +41:12:01.9 -- not an asteroid (will add it to exclusion list)
05:19:31.37 +41:08:13.6 -- not an asteroid (will add it to exclusion list)
05:40:17.56 +46:01:05.4 -- not an asteroid (will add it to exclusion list)
05:22:12.40 +41:06:52.8 -- not an asteroid (will add it to exclusion list)
05:20:04.97 +41:39:14.0 -- not an asteroid (will add it to exclusion list)
05:22:56.32 +40:57:00.2 -- not an asteroid (will add it to exclusion list)
05:28:01.16 +48:14:58.9 -- not an asteroid (will add it to exclusion list)
05:17:44.79 +41:17:54.0 -- not an asteroid (will add it to exclusion list)
05:20:41.60 +49:23:44.5 -- not an asteroid (will add it to exclusion list)
05:21:02.28 +40:59:50.8 -- not an asteroid (will add it to exclusion list)
05:47:22.10 +46:02:51.4 -- not an asteroid (will add it to exclusion list)
05:20:00.07 +41:39:11.7 -- not an asteroid (will add it to exclusion list)
05:20:56.82 +41:41:27.6 -- not an asteroid (will add it to exclusion list)
05:19:18.46 +41:43:23.0 -- not an asteroid (will add it to exclusion list)
05:18:48.90 +41:33:08.5 -- not an asteroid (will add it to exclusion list)
05:18:33.51 +40:55:58.4 -- not an asteroid (will add it to exclusion list)
05:18:19.07 +42:20:17.5 -- not an asteroid (will add it to exclusion list)
05:21:14.48 +41:05:09.5 -- not an asteroid (will add it to exclusion list)
05:18:47.20 +41:36:34.4 -- not an asteroid (will add it to exclusion list)
05:17:16.13 +41:16:54.2 -- not an asteroid (will add it to exclusion list)
05:17:45.94 +42:13:18.5 -- not an asteroid (will add it to exclusion list)
05:18:20.57 +41:53:19.0 -- not an asteroid (will add it to exclusion list)
05:20:34.96 +40:57:01.5 -- not an asteroid (will add it to exclusion list)
05:18:13.25 +41:29:51.2 -- not an asteroid (will add it to exclusion list)
06:12:44.60 +47:30:42.7 -- not an asteroid (will add it to exclusion list)
06:13:33.56 +48:03:18.0 -- not an asteroid (will add it to exclusion list)
06:01:16.84 +47:35:44.3 -- not an asteroid (will add it to exclusion list)
05:20:26.35 +42:15:37.0 -- not an asteroid (will add it to exclusion list)
05:22:46.02 +42:02:53.9 -- not an asteroid (will add it to exclusion list)
05:18:25.61 +42:09:12.0 -- not an asteroid (will add it to exclusion list)
05:25:13.31 +41:05:11.4 -- not an asteroid (will add it to exclusion list)
05:22:21.30 +41:29:28.5 -- not an asteroid (will add it to exclusion list)
05:17:39.42 +41:49:36.5 -- not an asteroid (will add it to exclusion list)
05:20:52.03 +41:45:37.0 -- not an asteroid (will add it to exclusion list)
05:22:15.12 +42:05:43.5 -- not an asteroid (will add it to exclusion list)
05:17:41.16 +41:50:36.2 -- not an asteroid (will add it to exclusion list)
05:18:08.85 +41:26:54.6 -- not an asteroid (will add it to exclusion list)
06:09:52.02 +46:34:27.5 -- not an asteroid (will add it to exclusion list)
05:17:17.06 +44:00:18.5 -- not an asteroid (will add it to exclusion list)
05:17:57.56 +41:23:11.9 -- not an asteroid (will add it to exclusion list)
05:20:07.62 +41:33:55.9 -- not an asteroid (will add it to exclusion list)
05:17:46.24 +41:44:25.9 -- not an asteroid (will add it to exclusion list)
05:20:55.85 +41:05:48.5 -- not an asteroid (will add it to exclusion list)
05:19:36.86 +41:50:09.1 -- not an asteroid (will add it to exclusion list)
05:21:07.49 +41:56:40.4 -- not an asteroid (will add it to exclusion list)
05:18:06.86 +41:54:42.3 -- not an asteroid (will add it to exclusion list)
05:19:10.19 +41:22:36.5 -- not an asteroid (will add it to exclusion list)
05:24:56.28 +41:22:19.1 -- not an asteroid (will add it to exclusion list)
05:23:17.15 +42:01:32.0 -- not an asteroid (will add it to exclusion list)
05:18:33.75 +42:05:19.0 -- not an asteroid (will add it to exclusion list)
05:18:31.68 +42:55:08.6 -- not an asteroid (will add it to exclusion list)
05:17:01.77 +43:09:35.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:16:32.32 +43:44:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:44.56 +42:12:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:52.88 +42:07:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:57.48 +42:27:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:01.76 +41:52:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:01.77 +43:09:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:02.25 +41:48:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:03.28 +41:28:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:03.54 +42:00:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:04.59 +41:49:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:04.64 +42:26:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:07.88 +42:00:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:08.60 +41:43:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:09.43 +41:50:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:13.09 +41:44:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:14.40 +41:46:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:15.02 +41:43:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:15.30 +42:00:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:15.84 +41:12:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:15.88 +42:10:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:16.13 +41:16:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:16.80 +41:55:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:17.06 +44:00:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:18.71 +42:19:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:18.76 +42:27:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:20.63 +41:54:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:21.25 +43:43:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.06 +41:29:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.15 +41:40:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.21 +41:36:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.75 +42:24:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.79 +41:57:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.91 +41:57:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:23.36 +42:32:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:23.79 +40:56:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:25.80 +41:01:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:27.03 +42:04:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:28.53 +41:13:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:28.80 +41:49:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:29.03 +41:47:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:29.48 +41:17:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:31.56 +42:08:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:32.96 +42:23:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:33.46 +41:45:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:36.05 +41:41:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:38.02 +41:40:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:38.65 +42:14:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:39.16 +41:50:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:39.42 +41:49:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:40.00 +41:57:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:41.16 +41:50:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:41.78 +41:24:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:41.79 +41:03:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:41.86 +41:12:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:42.33 +42:09:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:43.47 +41:02:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:43.48 +41:35:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:43.54 +41:23:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:43.68 +41:05:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:44.50 +42:11:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:44.62 +41:41:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:44.79 +41:17:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:45.72 +41:41:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:45.94 +42:13:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:46.24 +41:44:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:46.25 +41:26:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:48.68 +41:41:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:49.92 +41:19:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:50.18 +41:52:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:50.58 +40:59:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:51.67 +41:13:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:52.95 +41:57:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:56.22 +41:11:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:57.56 +41:23:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:57.69 +41:51:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:57.77 +41:10:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:58.28 +41:41:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:58.67 +41:54:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:59.26 +41:42:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:59.36 +42:12:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:00.23 +41:05:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:01.96 +41:23:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:03.55 +42:06:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:04.61 +44:13:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:06.86 +41:54:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:07.11 +41:46:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:08.85 +41:26:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:09.11 +42:18:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:09.63 +42:06:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:09.68 +42:30:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:09.76 +40:56:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:09.87 +41:34:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:11.62 +41:27:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:11.73 +41:06:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:13.00 +41:37:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:13.25 +41:29:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:13.49 +41:50:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:13.52 +41:41:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:13.74 +41:50:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:15.39 +41:28:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:19.07 +42:20:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:19.13 +41:00:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:20.57 +41:53:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:21.62 +41:34:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:22.38 +41:29:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:23.67 +41:28:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:24.57 +41:48:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:25.61 +42:09:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:25.87 +42:08:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:28.49 +43:23:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:30.28 +43:23:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:31.68 +42:55:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:33.43 +41:04:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:33.51 +40:55:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:33.75 +42:05:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:33.91 +42:17:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:34.48 +41:19:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:35.38 +41:27:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:36.21 +41:46:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:38.13 +42:14:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:42.48 +41:33:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:45.14 +42:03:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:47.20 +41:36:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:48.90 +41:33:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:52.23 +41:48:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:56.89 +41:23:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:59.13 +41:42:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:01.04 +41:43:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:01.33 +41:46:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:05.62 +41:12:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:09.37 +41:40:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:09.42 +41:18:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:09.52 +41:39:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:10.19 +41:22:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:17.13 +41:01:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:18.46 +41:43:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:19.10 +41:59:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:19.62 +40:59:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:22.67 +41:06:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:23.07 +41:17:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:26.45 +41:33:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:30.19 +41:56:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:30.54 +41:29:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:31.24 +41:15:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:31.37 +41:08:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:32.68 +41:34:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:33.37 +41:30:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:34.02 +41:42:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:34.56 +41:44:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:36.72 +41:02:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:36.85 +42:36:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:36.86 +41:50:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:37.57 +41:21:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:37.73 +41:47:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:39.30 +41:16:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:40.99 +41:28:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:41.69 +41:41:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:42.64 +41:26:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:43.62 +41:22:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:44.90 +41:25:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:45.11 +41:19:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:47.63 +40:57:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:51.14 +40:54:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:53.85 +41:09:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:56.49 +41:31:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:59.12 +40:55:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:00.07 +41:39:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:04.97 +41:39:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:05.17 +41:14:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:07.62 +41:33:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:09.00 +41:38:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:09.95 +41:28:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:12.06 +41:50:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:13.91 +41:33:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:26.35 +42:15:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:27.78 +41:00:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:28.44 +41:37:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:28.88 +41:41:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:29.97 +41:51:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:32.66 +41:09:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:34.14 +41:32:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:34.35 +41:18:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:34.96 +40:57:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:36.24 +41:26:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:37.17 +41:03:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:41.08 +43:25:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:41.60 +49:23:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:42.92 +40:54:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:46.01 +40:57:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:52.03 +41:45:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:53.49 +43:20:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:55.85 +41:05:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:56.82 +41:41:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:57.31 +41:19:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:59.01 +40:58:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:01.13 +41:24:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:02.28 +40:59:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:03.21 +41:27:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:03.45 +40:57:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:03.53 +41:02:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:04.81 +41:33:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:07.49 +41:56:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:07.55 +41:01:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:11.00 +41:07:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:11.83 +40:58:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:14.48 +41:05:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:16.64 +41:18:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:17.63 +41:12:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:19.27 +40:58:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:26.78 +41:09:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:27.30 +41:18:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:28.74 +41:03:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:35.75 +41:24:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:35.86 +41:17:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:43.91 +40:55:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:46.28 +41:06:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:46.41 +41:09:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:47.64 +41:19:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:48.20 +41:07:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:53.86 +41:14:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:56.13 +41:24:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:00.78 +41:12:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:02.87 +40:59:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:12.40 +41:06:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:15.07 +41:08:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:15.12 +42:05:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:21.30 +41:29:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:26.82 +41:02:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:38.68 +42:27:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:46.02 +42:02:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:56.32 +40:57:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:17.15 +42:01:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:31.04 +42:18:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:34.69 +41:13:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:56.28 +41:22:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:13.31 +41:05:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.73 +50:07:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.16 +48:14:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:45.51 +51:02:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:40.19 +48:17:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:17.56 +46:01:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:43.00 +48:20:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:53.04 +47:06:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:15.81 +43:29:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:22.10 +46:02:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.84 +47:35:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:41.39 +41:19:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:33.54 +43:09:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:52.02 +46:34:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:06.00 +41:55:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:44.60 +47:30:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:33.56 +48:03:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:36.27 +44:32:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:43.96 +44:42:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:03.79 +44:40:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:51.95 +43:32:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.97 +41:59:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:33.97 +49:51:14.5 -- 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)
05:16:32.32 +43:44:08.9 -- not a known variable star
05:16:44.56 +42:12:54.0 -- a known variable star
05:16:52.88 +42:07:31.6 -- a known variable star
05:16:57.48 +42:27:00.6 -- not a known variable star
05:17:01.76 +41:52:11.1 -- not a known variable star
05:17:01.77 +43:09:35.5 -- not a known variable star
05:17:02.25 +41:48:42.7 -- not a known variable star
05:17:03.28 +41:28:02.5 -- not a known variable star
05:17:03.54 +42:00:52.5 -- not a known variable star
05:17:04.59 +41:49:58.0 -- a known variable star
05:17:04.64 +42:26:01.3 -- not a known variable star
05:17:07.88 +42:00:29.7 -- not a known variable star
05:17:08.60 +41:43:48.8 -- not a known variable star
05:17:09.43 +41:50:12.7 -- not a known variable star
05:17:13.09 +41:44:46.8 -- not a known variable star
05:17:14.40 +41:46:08.7 -- not a known variable star
05:17:15.02 +41:43:32.7 -- not a known variable star
05:17:15.30 +42:00:41.2 -- not a known variable star
05:17:15.84 +41:12:38.4 -- not a known variable star
05:17:15.88 +42:10:20.7 -- a known variable star
05:17:16.13 +41:16:54.2 -- not a known variable star
05:17:16.80 +41:55:39.1 -- not a known variable star
05:17:17.06 +44:00:18.5 -- not a known variable star
05:17:18.71 +42:19:03.8 -- a known variable star
05:17:18.76 +42:27:03.9 -- not a known variable star
05:17:20.63 +41:54:56.5 -- a known variable star
05:17:21.25 +43:43:46.9 -- not a known variable star
05:17:22.06 +41:29:30.2 -- not a known variable star
05:17:22.15 +41:40:33.6 -- not a known variable star
05:17:22.21 +41:36:53.2 -- not a known variable star
05:17:22.75 +42:24:38.3 -- not a known variable star
05:17:22.79 +41:57:52.3 -- not a known variable star
05:17:22.91 +41:57:26.6 -- not a known variable star
05:17:23.36 +42:32:04.8 -- not a known variable star
05:17:23.79 +40:56:49.1 -- a known variable star
05:17:25.80 +41:01:31.9 -- not a known variable star
05:17:27.03 +42:04:46.0 -- not a known variable star
05:17:28.53 +41:13:52.7 -- not a known variable star
05:17:28.80 +41:49:34.7 -- not a known variable star
05:17:29.03 +41:47:23.6 -- not a known variable star
05:17:29.48 +41:17:17.1 -- not a known variable star
05:17:31.56 +42:08:57.1 -- a known variable star
05:17:32.96 +42:23:23.0 -- not a known variable star
05:17:33.46 +41:45:08.1 -- not a known variable star
05:17:36.05 +41:41:02.4 -- not a known variable star
05:17:38.02 +41:40:02.0 -- a known variable star
05:17:38.65 +42:14:41.9 -- not a known variable star
05:17:39.16 +41:50:01.0 -- a known variable star
05:17:39.42 +41:49:36.5 -- a known variable star
05:17:40.00 +41:57:06.9 -- not a known variable star
05:17:41.16 +41:50:36.2 -- not a known variable star
05:17:41.78 +41:24:12.1 -- not a known variable star
05:17:41.79 +41:03:14.7 -- a known variable star
05:17:41.86 +41:12:31.6 -- not a known variable star
05:17:42.33 +42:09:26.8 -- a known variable star
05:17:43.47 +41:02:37.1 -- not a known variable star
05:17:43.48 +41:35:28.2 -- not a known variable star
05:17:43.54 +41:23:54.6 -- a known variable star
05:17:43.68 +41:05:44.2 -- a known variable star
05:17:44.50 +42:11:19.3 -- not a known variable star
05:17:44.62 +41:41:19.9 -- not a known variable star
05:17:44.79 +41:17:54.0 -- not a known variable star
05:17:45.72 +41:41:57.8 -- not a known variable star
05:17:45.94 +42:13:18.5 -- not a known variable star
05:17:46.24 +41:44:25.9 -- not a known variable star
05:17:46.25 +41:26:53.2 -- not a known variable star
05:17:48.68 +41:41:34.0 -- a known variable star
05:17:49.92 +41:19:53.8 -- not a known variable star
05:17:50.18 +41:52:05.9 -- a known variable star
05:17:50.58 +40:59:14.2 -- not a known variable star
05:17:51.67 +41:13:13.5 -- not a known variable star
05:17:52.95 +41:57:10.7 -- a known variable star
05:17:56.22 +41:11:56.5 -- a known variable star
05:17:57.56 +41:23:11.9 -- not a known variable star
05:17:57.69 +41:51:47.5 -- not a known variable star
05:17:57.77 +41:10:44.5 -- not a known variable star
05:17:58.28 +41:41:03.5 -- not a known variable star
05:17:58.67 +41:54:50.1 -- not a known variable star
05:17:59.26 +41:42:14.4 -- not a known variable star
05:17:59.36 +42:12:01.2 -- not a known variable star
05:18:00.23 +41:05:42.0 -- a known variable star
05:18:01.96 +41:23:18.1 -- not a known variable star
05:18:03.55 +42:06:18.5 -- not a known variable star
05:18:04.61 +44:13:03.0 -- not a known variable star
05:18:06.86 +41:54:42.3 -- not a known variable star
05:18:07.11 +41:46:17.0 -- not a known variable star
05:18:08.85 +41:26:54.6 -- not a known variable star
05:18:09.11 +42:18:27.1 -- not a known variable star
05:18:09.63 +42:06:05.5 -- not a known variable star
05:18:09.68 +42:30:21.8 -- a known variable star
05:18:09.76 +40:56:38.3 -- not a known variable star
05:18:09.87 +41:34:39.5 -- not a known variable star
05:18:11.62 +41:27:00.6 -- not a known variable star
05:18:11.73 +41:06:05.5 -- not a known variable star
05:18:13.00 +41:37:19.8 -- not a known variable star
05:18:13.25 +41:29:51.2 -- not a known variable star
05:18:13.49 +41:50:58.2 -- a known variable star
05:18:13.52 +41:41:03.5 -- a known variable star
05:18:13.74 +41:50:13.8 -- not a known variable star
05:18:15.39 +41:28:35.9 -- not a known variable star
05:18:19.07 +42:20:17.5 -- not a known variable star
05:18:19.13 +41:00:06.2 -- a known variable star
05:18:20.57 +41:53:19.0 -- not a known variable star
05:18:21.62 +41:34:57.8 -- not a known variable star
05:18:22.38 +41:29:29.8 -- not a known variable star
05:18:23.67 +41:28:28.5 -- not a known variable star
05:18:24.57 +41:48:04.5 -- not a known variable star
05:18:25.61 +42:09:12.0 -- not a known variable star
05:18:25.87 +42:08:49.6 -- not a known variable star
05:18:28.49 +43:23:12.9 -- not a known variable star
05:18:30.28 +43:23:29.8 -- a known variable star
05:18:31.68 +42:55:08.6 -- not a known variable star
05:18:33.43 +41:04:56.1 -- not a known variable star
05:18:33.51 +40:55:58.4 -- a known variable star
05:18:33.75 +42:05:19.0 -- not a known variable star
05:18:33.91 +42:17:09.8 -- a known variable star
05:18:34.48 +41:19:31.6 -- not a known variable star
05:18:35.38 +41:27:42.3 -- not a known variable star
05:18:36.21 +41:46:23.8 -- not a known variable star
05:18:38.13 +42:14:06.1 -- a known variable star
05:18:42.48 +41:33:09.0 -- a known variable star
05:18:45.14 +42:03:00.3 -- not a known variable star
05:18:47.20 +41:36:34.4 -- a known variable star
05:18:48.90 +41:33:08.5 -- a known variable star
05:18:52.23 +41:48:27.7 -- not a known variable star
05:18:56.89 +41:23:06.9 -- a known variable star
05:18:59.13 +41:42:18.2 -- not a known variable star
05:19:01.04 +41:43:45.8 -- not a known variable star
05:19:01.33 +41:46:25.8 -- not a known variable star
05:19:05.62 +41:12:55.9 -- a known variable star
05:19:09.37 +41:40:20.0 -- not a known variable star
05:19:09.42 +41:18:59.1 -- not a known variable star
05:19:09.52 +41:39:36.5 -- not a known variable star
05:19:10.19 +41:22:36.5 -- not a known variable star
05:19:17.13 +41:01:57.9 -- not a known variable star
05:19:18.46 +41:43:23.0 -- a known variable star
05:19:19.10 +41:59:23.2 -- not a known variable star
05:19:19.62 +40:59:12.5 -- not a known variable star
05:19:22.67 +41:06:10.6 -- not a known variable star
05:19:23.07 +41:17:39.0 -- not a known variable star
05:19:26.45 +41:33:40.0 -- not a known variable star
05:19:30.19 +41:56:21.0 -- not a known variable star
05:19:30.54 +41:29:14.0 -- not a known variable star
05:19:31.24 +41:15:46.4 -- not a known variable star
05:19:31.37 +41:08:13.6 -- a known variable star
05:19:32.68 +41:34:44.4 -- not a known variable star
05:19:33.37 +41:30:24.1 -- not a known variable star
05:19:34.02 +41:42:04.8 -- a known variable star
05:19:34.56 +41:44:04.0 -- not a known variable star
05:19:36.72 +41:02:30.2 -- a known variable star
05:19:36.85 +42:36:22.3 -- not a known variable star
05:19:36.86 +41:50:09.1 -- not a known variable star
05:19:37.57 +41:21:38.6 -- a known variable star
05:19:37.73 +41:47:12.4 -- not a known variable star
05:19:39.30 +41:16:19.8 -- not a known variable star
05:19:40.99 +41:28:15.9 -- a known variable star
05:19:41.69 +41:41:45.5 -- not a known variable star
05:19:42.64 +41:26:17.8 -- not a known variable star
05:19:43.62 +41:22:52.2 -- not a known variable star
05:19:44.90 +41:25:28.8 -- not a known variable star
05:19:45.11 +41:19:52.9 -- not a known variable star
05:19:47.63 +40:57:28.0 -- a known variable star
05:19:51.14 +40:54:04.5 -- not a known variable star
05:19:53.85 +41:09:16.5 -- not a known variable star
05:19:56.49 +41:31:31.5 -- not a known variable star
05:19:59.12 +40:55:10.5 -- not a known variable star
05:20:00.07 +41:39:11.7 -- a known variable star
05:20:04.97 +41:39:14.0 -- a known variable star
05:20:05.17 +41:14:24.8 -- not a known variable star
05:20:07.62 +41:33:55.9 -- not a known variable star
05:20:09.00 +41:38:29.3 -- not a known variable star
05:20:09.95 +41:28:55.1 -- a known variable star
05:20:12.06 +41:50:45.1 -- not a known variable star
05:20:13.91 +41:33:22.4 -- not a known variable star
05:20:26.35 +42:15:37.0 -- not a known variable star
05:20:27.78 +41:00:57.8 -- not a known variable star
05:20:28.44 +41:37:05.0 -- not a known variable star
05:20:28.88 +41:41:24.3 -- a known variable star
05:20:29.97 +41:51:22.7 -- not a known variable star
05:20:32.66 +41:09:01.5 -- a known variable star
05:20:34.14 +41:32:12.4 -- not a known variable star
05:20:34.35 +41:18:00.6 -- not a known variable star
05:20:34.96 +40:57:01.5 -- a known variable star
05:20:36.24 +41:26:10.9 -- a known variable star
05:20:37.17 +41:03:53.1 -- not a known variable star
05:20:41.08 +43:25:39.7 -- a known variable star
05:20:41.60 +49:23:44.5 -- not a known variable star
05:20:42.92 +40:54:42.0 -- not a known variable star
05:20:46.01 +40:57:08.7 -- not a known variable star
05:20:52.03 +41:45:37.0 -- not a known variable star
05:20:53.49 +43:20:16.7 -- a known variable star
05:20:55.85 +41:05:48.5 -- not a known variable star
05:20:56.82 +41:41:27.6 -- a known variable star
05:20:57.31 +41:19:28.7 -- a known variable star
05:20:59.01 +40:58:25.8 -- not a known variable star
05:21:01.13 +41:24:15.2 -- a known variable star
05:21:02.28 +40:59:50.8 -- not a known variable star
05:21:03.21 +41:27:00.1 -- not a known variable star
05:21:03.45 +40:57:03.1 -- not a known variable star
05:21:03.53 +41:02:20.3 -- not a known variable star
05:21:04.81 +41:33:48.6 -- not a known variable star
05:21:07.49 +41:56:40.4 -- not a known variable star
05:21:07.55 +41:01:50.2 -- not a known variable star
05:21:11.00 +41:07:23.0 -- not a known variable star
05:21:11.83 +40:58:15.5 -- not a known variable star
05:21:14.48 +41:05:09.5 -- not a known variable star
05:21:16.64 +41:18:05.5 -- not a known variable star
05:21:17.63 +41:12:01.4 -- not a known variable star
05:21:19.27 +40:58:22.2 -- a known variable star
05:21:26.78 +41:09:41.1 -- not a known variable star
05:21:27.30 +41:18:34.6 -- not a known variable star
05:21:28.74 +41:03:43.8 -- a known variable star
05:21:35.75 +41:24:39.2 -- not a known variable star
05:21:35.86 +41:17:58.9 -- a known variable star
05:21:43.91 +40:55:58.4 -- not a known variable star
05:21:46.28 +41:06:10.3 -- not a known variable star
05:21:46.41 +41:09:51.6 -- not a known variable star
05:21:47.64 +41:19:19.6 -- not a known variable star
05:21:48.20 +41:07:18.4 -- not a known variable star
05:21:53.86 +41:14:46.1 -- not a known variable star
05:21:56.13 +41:24:48.4 -- a known variable star
05:22:00.78 +41:12:01.9 -- not a known variable star
05:22:02.87 +40:59:16.6 -- not a known variable star
05:22:12.40 +41:06:52.8 -- not a known variable star
05:22:15.07 +41:08:09.0 -- not a known variable star
05:22:15.12 +42:05:43.5 -- a known variable star
05:22:21.30 +41:29:28.5 -- a known variable star
05:22:26.82 +41:02:54.2 -- not a known variable star
05:22:38.68 +42:27:33.6 -- a known variable star
05:22:46.02 +42:02:53.9 -- a known variable star
05:22:56.32 +40:57:00.2 -- not a known variable star
05:23:17.15 +42:01:32.0 -- not a known variable star
05:24:31.04 +42:18:55.1 -- not a known variable star
05:24:34.69 +41:13:46.4 -- not a known variable star
05:24:56.28 +41:22:19.1 -- a known variable star
05:25:13.31 +41:05:11.4 -- not a known variable star
05:27:04.73 +50:07:23.2 -- a known variable star
05:28:01.16 +48:14:58.9 -- a known variable star
05:31:45.51 +51:02:32.1 -- a known variable star
05:33:40.19 +48:17:45.2 -- not a known variable star
05:40:17.56 +46:01:05.4 -- not a known variable star
05:40:43.00 +48:20:10.6 -- not a known variable star
05:43:53.04 +47:06:14.7 -- not a known variable star
05:47:15.81 +43:29:09.2 -- not a known variable star
05:47:22.10 +46:02:51.4 -- not a known variable star
06:01:16.84 +47:35:44.3 -- not a known variable star
06:08:41.39 +41:19:36.9 -- a known variable star
06:09:33.54 +43:09:03.8 -- not a known variable star
06:09:52.02 +46:34:27.5 -- a known variable star
06:11:06.00 +41:55:49.6 -- not a known variable star
06:12:44.60 +47:30:42.7 -- not a known variable star
06:13:33.56 +48:03:18.0 -- not a known variable star
06:16:36.27 +44:32:55.4 -- a known variable star
06:16:43.96 +44:42:40.5 -- not a known variable star
06:24:03.79 +44:40:33.8 -- not a known variable star
06:24:51.95 +43:32:25.8 -- a known variable star
06:26:19.97 +41:59:11.2 -- not a known variable star
06:48:33.97 +49:51:14.5 -- not a known variable star
Found 190 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
258 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 258 (excluding asteroids and hot pixels, 190 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)2461153.68980222 -observatory V36
00:47:45.30 +02:22:53.1 Mercury (-0.3mag)
03:44:16.30 +20:20:31.9 Venus (-3.9mag)
00:38:13.85 +03:05:50.1 Mars (1.2mag)
07:16:09.91 +22:40:15.0 Jupiter (-2.1mag)
00:32:20.67 +01:08:34.9 Saturn (0.9mag)
03:49:15.21 +19:52:25.7 Uranus (5.8mag)
00:11:45.55 -00:09:36.3 Neptune (7.8mag)
20:34:01.09 -22:53:07.1 Pluto (14.5mag)
07:29:20.66 +25:08:56.4 Moon (-10.1mag)
-rw-r--r-- 1 apache apache 363 Apr 22 23:36 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461153.68980222:
07:16:11.15 +22:40:14.7 Io (5.8mag)
07:16:14.61 +22:40:07.1 Europa (6.0mag)
07:16:27.54 +22:39:33.4 Ganymede (5.4mag)
07:15:40.66 +22:41:12.4 Callisto (6.6mag)
07:19:09.72 +22:24:44.7 Himalia (15.4mag)
07:16:12.04 +22:40:12.0 Thebe (16.3mag)
07:19:29.36 +22:55:00.6 Elara (17.3mag)
07:15:32.05 +23:16:29.6 Pasiphae (17.5mag)
07:24:19.42 +22:38:54.9 Carme (18.6mag)
00:32:18.94 +01:08:26.6 Titan (8.8mag)
00:32:22.91 +01:08:48.6 Rhea (10.1mag)
00:31:51.99 +01:07:36.8 Iapetus (11.5mag)
00:32:10.08 +01:08:44.0 Hyperion (14.8mag)
00:33:51.60 +01:16:34.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 22 23:36 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461153.68980222:
16:06:45.51 -20:51:29.1 JWST
18:50:47.11 +22:12:13.5 Chandra
17:45:24.16 -42:11:51.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 22 23:36 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461153.68980222 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:36:29.35 +30:48:24.1 18.0mag P/2009 WX51 (Catalina)
18:54:22.97 -29:13:15.7 13.8mag P/2010 H2 (Vales)
05:12:06.88 -69:20:12.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:34:08.13 +31:29:22.8 17.3mag C/2017 K2 (PANSTARRS)
17:29:27.93 +11:22:58.6 17.7mag C/2021 G2 (ATLAS)
23:11:57.02 +29:31:40.2 17.1mag C/2022 E2 (ATLAS)
04:37:42.79 +26:13:35.5 16.1mag C/2022 N2 (PANSTARRS)
09:05:17.84 +32:01:46.5 16.3mag C/2022 QE78 (ATLAS)
08:32:25.94 +00:34:45.4 17.4mag C/2022 R6 (PANSTARRS)
18:51:44.13 +19:07:15.6 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:09.86 -11:24:55.9 17.5mag P/2023 B1 (PANSTARRS)
09:04:42.61 -10:46:09.3 17.7mag C/2023 F3 (ATLAS)
22:00:51.12 +63:20:56.1 17.6mag C/2023 H5 (Lemmon)
19:12:07.63 -03:52:49.8 14.1mag C/2023 R1 (PANSTARRS)
21:07:32.39 +86:55:16.2 17.8mag C/2023 X2 (Lemmon)
06:21:55.54 +63:30:01.6 17.2mag C/2024 A1 (ATLAS)
05:28:07.54 +20:27:31.9 11.5mag C/2024 E1 (Wierzchos)
16:14:22.89 +07:33:24.9 17.3mag C/2024 G6 (ATLAS)
20:22:28.05 +17:16:13.6 14.5mag C/2024 J3 (ATLAS)
03:32:56.39 -21:19:17.9 16.3mag C/2024 T5 (ATLAS)
05:22:58.18 +43:34:09.4 17.7mag C/2025 J1 (Borisov)
13:09:46.11 +49:15:17.7 15.5mag C/2025 L1 (ATLAS)
03:37:01.41 -27:23:02.9 17.9mag C/2025 Q3 (ATLAS)
01:23:14.46 +12:57:31.9 7.8mag C/2025 R3 (PANSTARRS)
12:51:04.34 +03:25:40.5 17.4mag C/2025 Y1 (ATLAS)
04:15:53.99 +02:04:09.4 15.1mag C/2026 A1 (MAPS)
00:19:21.88 +38:26:51.6 14.8mag C/2026 B2 (Sun-Gao)
18:56:53.22 -09:19:36.5 11.4mag 10P/Tempel
14:50:30.55 +02:23:06.3 14.6mag 24P/Schaumasse
11:01:07.59 -01:18:44.0 15.7mag 29P/Schwassmann-Wachmann
10:37:51.15 -03:34:51.6 17.1mag 43P/Wolf-Harrington
01:59:50.31 +18:41:51.9 17.3mag 47P/Ashbrook-Jackson
07:24:24.07 +35:26:15.9 17.0mag 63P/Wild
23:38:03.50 -10:36:26.4 15.7mag 65P/Gunn
04:22:52.59 +23:37:20.4 15.9mag 76P/West-Kohoutek-Ikemura
01:21:36.03 +09:37:31.0 14.2mag 78P/Gehrels
23:24:17.36 -07:15:58.1 14.7mag 88P/Howell
02:31:05.57 +22:29:40.8 15.0mag 93P/Lovas
05:08:44.18 +32:38:29.9 16.1mag 123P/West-Hartley
08:37:25.39 +35:03:13.8 16.2mag 124P/Mrkos
02:44:25.62 +15:09:22.7 16.4mag 128P/Shoemaker-Holt
03:01:42.41 +15:20:17.4 17.5mag 131P/Mueller
02:04:33.29 +15:30:47.5 10.5mag 141P/Machholz
02:12:18.02 +07:31:42.0 10.5mag 141P-A/Machholz
00:54:38.67 +03:16:09.5 12.0mag 141P-D/Machholz
02:42:56.23 +09:15:16.9 17.9mag 141P-I/Machholz
01:22:33.14 +02:06:21.7 15.0mag 162P/SidingSpring
14:38:50.94 +00:34:47.8 17.9mag 210P/Christensen
21:58:40.96 -09:44:18.8 17.8mag 218P/LINEAR
17:17:24.65 -13:03:13.7 16.1mag 235P/LINEAR
05:50:13.02 +35:10:40.0 16.9mag 240P/NEAT
07:42:20.95 -04:25:46.8 17.8mag 242P/Spahr
22:34:54.52 -18:58:52.8 17.7mag 260P/McNaught
02:13:09.37 +22:15:13.9 17.9mag 295P/LINEAR
15:39:33.07 +07:25:58.1 17.5mag 391P/Kowalski
07:37:15.54 +21:22:20.4 17.7mag 450P/LONEOS
05:46:33.96 +44:36:45.8 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 22 23:36 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
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
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
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
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
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
-rw-r--r-- 1 apache apache 188K Apr 22 23:36 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:37:46.128 -00:10:27.29 AT 2026jqy 2026-04-15.44 19.9423
21:22:43.135 +01:34:03.91 AT 2026jqx 2026-04-15.50 19.506
20:20:49.879 -54:50:37.33 AT 2026jqw 2026-04-15.38 18.428
14:18:06.700 +18:27:11.82 AT 2026jqv 2026-04-15.09 18.593
05:54:56.359 -64:02:05.45 AT 2026jqu 2026-04-15.74 19.448
23:56:40.308 -79:35:41.95 AT 2026jqt 2026-04-15.38 18.924
04:07:29.216 -53:22:08.08 AT 2026jqs 2026-04-15.75 18.414
15:43:49.348 +30:31:32.85 AT 2026jqr 2026-04-15.07 19.396
10:01:06.186 +12:53:37.52 AT 2026jqq 2026-04-14.00 19.168
21:41:55.797 +08:42:01.92 AT 2026jqp 2026-04-15.51 19.6758
20:30:05.017 +14:09:09.48 AT 2026jqo 2026-04-13.20 19.78
18:56:45.384 +43:09:18.15 AT 2026jqn 2026-04-14.23 18.62
12:34:36.583 +07:30:35.59 AT 2026jqm 2026-04-15.29 22.3871
21:15:43.547 +02:04:36.79 AT 2026jql 2026-04-10.51 18.5787
21:17:35.104 -09:31:48.68 AT 2026jqk 2026-04-08.51 19.2234
23:17:19.653 +25:48:48.77 AT 2026jqj 2026-04-10.52 19.017
21:35:46.821 -63:54:12.77 SN 2026jqi 2026-04-15.38 18.808
14:55:11.021 +13:27:58.31 AT 2026jqh 2026-04-12.04 19.94
17:06:10.839 +21:24:48.24 AT 2026jqg 2026-04-12.16 19.7
16:45:24.718 -07:18:03.25 AT 2026jqf 2026-04-10.44 20.4521
-rw-r--r-- 1 apache apache 30K Apr 22 23:36 tns_transients_list.txt
