This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 13.57 06:14:02.99 +50:52:47.6
163.11319 15.22216 galactic Aur Second-epoch detections are separated by 0.8" and 4.8 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 | 06:14:02.99 +50:52:47.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.406+/-0.037 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:14:02.99 +50:52:47.6: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:14:02.99 +50:52:47.6: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 13.57CV 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 22.1528 2461152.6528 13.32 05:45:51.93 +50:23:48.2
161.47106 11.02324 galactic Aur Second-epoch detections are separated by 1.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:45:51.93 +50:23:48.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.557+/-0.031 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:45:51.93 +50:23:48.2: 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 05:45:51.93 +50:23:48.2: 14.22 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 13.32CV 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 22.1528 2461152.6528 12.90 05:53:45.75 +44:06:44.9
167.69987 9.10722 galactic Aur Second-epoch detections are separated by 1.4" and 4.8 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 J088.4375+44.1163 | 05:53:45.75 +44:06:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.455+/-0.028 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:53:45.75 +44:06:44.9: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:53:45.75 +44:06:44.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 J088.4375+44.1163,2461152.6528,12.90,0.05,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 J088.4375+44.1163 20260422.1528 12.90CV 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 22.1528 2461152.6528 12.90 05:46:42.28 +41:24:56.8
169.40707 6.63950 galactic Aur Second-epoch detections are separated by 0.5" and 4.7 pix
The object was found in VSX 1" Gaia DR3 192682064081902336
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.040 G 14.120 G 0.064870100000 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 05:46:42.28 +41:24:56.8: 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 05:46:42.28 +41:24:56.8: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192682064081902336,2461152.6528,12.90,0.05,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 192682064081902336 20260422.1528 12.90CV 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 22.1528 2461152.6528 12.50 05:16:30.05 +50:58:24.5
158.47077 7.39283 galactic Aur Second-epoch detections are separated by 3.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:16:30.05 +50:58:24.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:16:30.05 +50:58:24.5: 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 05:16:30.05 +50:58:24.5: 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
target,2461152.6528,12.50,0.05,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
target 20260422.1528 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.68 05:28:04.06 +49:28:28.7
160.76606 8.09655 galactic Aur Second-epoch detections are separated by 1.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.0152+49.4731 | 05:28:04.06 +49:28:28.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:28:04.06 +49:28:28.7: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:28:04.06 +49:28:28.7: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 J082.0152+49.4731,2461152.6528,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.0152+49.4731 20260422.1528 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 11.51 05:46:26.50 +47:55:01.2
163.70865 9.87608 galactic Aur Second-epoch detections are separated by 0.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 209974903788049920 | 05:46:26.64 +47:55:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:46:26.50 +47:55:01.2: 13.73 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:46:26.50 +47:55:01.2: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 209974903788049920,2461152.6528,11.51,0.05,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
Gaia DR3 209974903788049920 20260422.1528 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 11.79 05:49:29.01 +44:16:19.6
167.17677 8.51851 galactic Aur Second-epoch detections are separated by 0.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 196564783236506368 | 05:49:28.71 +44:16:56.4 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 1929BHarO.871...14C BD+44 1291 J-Ks=0.294+/-0.028 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:49:29.01 +44:16:19.6: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:49:29.01 +44:16:19.6: 12.75 +/- 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
Gaia DR3 196564783236506368,2461152.6528,11.79,0.05,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 196564783236506368 20260422.1528 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 22.1528 2461152.6528 11.93 06:21:48.26 +46:46:31.0
167.52847 14.69487 galactic Aur Second-epoch detections are separated by 0.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.4512+46.7771 | 06:21:48.26 +46:46:31.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:21:48.26 +46:46:31.0: 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 06:21:48.26 +46:46:31.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 J095.4512+46.7771,2461152.6528,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.4512+46.7771 20260422.1528 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 11.79 05:29:45.61 +49:44:06.0
160.69423 8.46793 galactic Aur Second-epoch detections are separated by 2.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.4263+49.7435 | 05:29:42.42 +49:44:13.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.893+/-0.025 (M)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:29:45.61 +49:44:06.0: 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 05:29:45.61 +49:44:06.0: 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 J082.4263+49.7435,2461152.6528,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.4263+49.7435 20260422.1528 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 22.1528 2461152.6528 11.90 05:29:21.98 +51:11:31.1
159.41602 9.19692 galactic Aur Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 261967239550603520 | 05:29:20.71 +51:12:00.9 (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 05:29:21.98 +51:11:31.1: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:29:21.98 +51:11:31.1: 12.89 +/- 0.02 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 261967239550603520,2461152.6528,11.90,0.05,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 261967239550603520 20260422.1528 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 22.1528 2461152.6528 11.96 05:25:48.82 +43:15:17.9
165.77802 4.35227 galactic Aur Second-epoch detections are separated by 2.4" and 4.3 pix
The object was found in VSX21" Gaia DR3 195701735329132160
Type: ROT
# Max. Min./Amp. JD0 Period
15.420 G 15.450 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 05:25:48.82 +43:15:17.9: 12.58 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:25:48.82 +43:15:17.9: 12.97 +/- 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 195701735329132160,2461152.6528,11.96,0.05,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 195701735329132160 20260422.1528 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 22.1528 2461152.6528 11.98 05:42:07.70 +50:04:31.5
161.45117 10.34503 galactic Aur Second-epoch detections are separated by 2.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 214356977317828864 | 05:42:06.70 +50:04:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-0.025 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:42:07.70 +50:04:31.5: 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 05:42:07.70 +50:04:31.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 214356977317828864,2461152.6528,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214356977317828864 20260422.1528 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 22.1528 2461152.6528 11.99 05:40:02.66 +50:02:05.9
161.31430 10.03619 galactic Aur Second-epoch detections are separated by 2.9" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.0114+50.0334 | 05:40:02.66 +50:02:05.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.245+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:40:02.66 +50:02:05.9: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:40:02.66 +50:02:05.9: 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
ATO J085.0114+50.0334,2461152.6528,11.99,0.05,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 J085.0114+50.0334 20260422.1528 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 22.1528 2461152.6528 12.12 05:48:04.13 +43:19:50.6
167.87105 7.82635 galactic Aur Second-epoch detections are separated by 0.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.0101+43.3293 | 05:48:00.35 +43:19:56.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.416+/-0.029 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:48:04.13 +43:19:50.6: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:48:04.13 +43:19:50.6: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 J087.0101+43.3293,2461152.6528,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.0101+43.3293 20260422.1528 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.49 06:26:19.86 +41:59:11.2
172.36999 13.45649 galactic Aur Second-epoch detections are separated by 1.2" and 5.1 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 | 06:26:19.86 +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 06:26:19.86 +41:59:11.2: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:26:19.86 +41:59:11.2: 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,2461152.6528,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.69 06:47:21.13 +48:12:02.0
167.82597 19.22952 galactic Aur Second-epoch detections are separated by 1.2" and 5.0 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 | 06:47:21.13 +48:12:02.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.333+/-0.035 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:47:21.13 +48:12:02.0: 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 06:47:21.13 +48:12:02.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461152.6528,12.69,0.05,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 20260422.1528 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 22.1528 2461152.6528 12.44 05:38:51.13 +41:49:43.2
168.28701 5.59848 galactic Aur Second-epoch detections are separated by 1.6" and 4.9 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 J084.7132+41.8303 | 05:38:51.13 +41:49:43.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:38:51.13 +41:49:43.2: 13.56 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:38:51.13 +41:49:43.2: 13.30 +/- 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
ATO J084.7132+41.8303,2461152.6528,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.7132+41.8303 20260422.1528 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.64 06:01:40.60 +44:57:46.8
167.62415 10.75236 galactic Aur Second-epoch detections are separated by 2.1" and 4.9 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 | 06:01:40.60 +44:57:46.8 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.029 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:01:40.60 +44:57:46.8: 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 06:01:40.60 +44:57:46.8: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461152.6528,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.68 05:38:24.43 +42:59:47.8
167.24561 6.14409 galactic Aur Second-epoch detections are separated by 1.9" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J084.6086+42.9942 | 05:38:24.43 +42:59:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7IV (LAMOST DR5) J-Ks=0.432+/-0.034 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:38:24.43 +42:59:47.8: 13.44 +/- 0.10 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:38:24.43 +42:59:47.8: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 J084.6086+42.9942,2461152.6528,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.6086+42.9942 20260422.1528 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.90 06:20:04.37 +46:37:59.6
167.53591 14.36586 galactic Aur Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:20:04.37 +46:37:59.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.308+/-0.033 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:20:04.37 +46:37:59.6: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:20:04.37 +46:37:59.6: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461152.6528,12.90,0.05,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 20260422.1528 12.90CV 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 22.1528 2461152.6528 12.66 05:27:26.07 +44:48:51.3
164.63651 5.45803 galactic Aur Second-epoch detections are separated by 2.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:27:26.07 +44:48:51.3 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.163+/-0.031 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:27:26.07 +44:48:51.3: 13.55 +/- 0.10 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:27:26.07 +44:48:51.3: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461152.6528,12.66,0.05,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 20260422.1528 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.64 05:28:11.73 +43:27:55.0
165.84262 4.82924 galactic Aur Second-epoch detections are separated by 0.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.0489+43.4659 | 05:28:14.53 +43:28:03.1 (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 05:28:11.73 +43:27:55.0: 13.77 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:28:11.73 +43:27:55.0: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J082.0489+43.4659,2461152.6528,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.0489+43.4659 20260422.1528 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.86 06:25:49.04 +48:15:43.3
166.39819 15.91178 galactic Aur Second-epoch detections are separated by 2.5" and 5.0 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 967525667862574848 | 06:25:52.69 +48:16:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.034 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:25:49.04 +48:15:43.3: 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 06:25:49.04 +48:15:43.3: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 967525667862574848,2461152.6528,12.86,0.05,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 967525667862574848 20260422.1528 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 22.1528 2461152.6528 12.89 05:54:13.34 +47:53:38.5
164.37573 11.00318 galactic Aur Second-epoch detections are separated by 1.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 210193191206491904 | 05:54:10.75 +47:53:19.9 (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 05:54:13.34 +47:53:38.5: 14.04 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:54:13.34 +47:53:38.5: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210193191206491904,2461152.6528,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210193191206491904 20260422.1528 12.89CV 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 22.1528 2461152.6528 12.62 05:20:50.94 +44:04:37.2
164.59039 4.07138 galactic Aur Second-epoch detections are separated by 2.4" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 207620613173739776 | 05:20:47.43 +44:04:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.221+/-0.040 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:20:50.94 +44:04:37.2: 13.74 +/- 0.14 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:20:50.94 +44:04:37.2: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 207620613173739776,2461152.6528,12.62,0.05,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 207620613173739776 20260422.1528 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 12.84 06:02:32.13 +48:11:24.3
164.77007 12.37035 galactic Aur Second-epoch detections are separated by 0.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.6351+48.1884 | 06:02:32.13 +48:11:24.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.647+/-0.035 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:02:32.13 +48:11:24.3: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:02:32.13 +48:11:24.3: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 J090.6351+48.1884,2461152.6528,12.84,0.05,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 J090.6351+48.1884 20260422.1528 12.84CV 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 22.1528 2461152.6528 12.96 06:12:44.90 +47:30:43.0
166.17236 13.60648 galactic Aur Second-epoch detections are separated by 1.1" and 4.9 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 968792687512124800 | 06:12:42.84 +47:30:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.388+/-0.032 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:12:44.90 +47:30:43.0: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:12:44.90 +47:30:43.0: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 968792687512124800,2461152.6528,12.96,0.05,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 968792687512124800 20260422.1528 12.96CV 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 22.1528 2461152.6528 12.81 05:31:42.96 +44:43:23.8
165.12986 6.04522 galactic Aur Second-epoch detections are separated by 3.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J053146.43+444302.5 | 05:31:46.43 +44:43:02.5 (Gaia DR3) | SR (local) | 2458232.61300 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:31:42.96 +44:43:23.8: 13.59 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:31:42.96 +44:43:23.8: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053146.43+444302.5,2461152.6528,12.81,0.05,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
ASASSN-V J053146.43+444302.5 20260422.1528 12.81CV 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 22.1528 2461152.6528 12.72 05:30:45.55 +43:28:05.8
166.09570 5.22018 galactic Aur Second-epoch detections are separated by 1.5" and 4.8 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 J082.6900+43.4677 | 05:30:45.55 +43:28:05.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.377+/-0.033 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:30:45.55 +43:28:05.8: 13.41 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:30:45.55 +43:28:05.8: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 J082.6900+43.4677,2461152.6528,12.72,0.05,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 J082.6900+43.4677 20260422.1528 12.72CV 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 22.1528 2461152.6528 12.70 05:35:29.73 +45:58:09.6
164.42762 7.27285 galactic Aur Second-epoch detections are separated by 2.9" and 4.9 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 209704634383239936 | 05:35:31.85 +45:57:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.038 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:35:29.73 +45:58:09.6: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:35:29.73 +45:58:09.6: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 209704634383239936,2461152.6528,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209704634383239936 20260422.1528 12.70CV 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 22.1528 2461152.6528 12.89 05:35:43.50 +44:16:09.7
165.90075 6.40554 galactic Aur Second-epoch detections are separated by 0.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.9541+44.2620 | 05:35:46.07 +44:15:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8III 1928MeUpp..37....1S BD+44 1243
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:35:43.50 +44:16:09.7: 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 05:35:43.50 +44:16:09.7: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 J083.9541+44.2620,2461152.6528,12.89,0.05,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 J083.9541+44.2620 20260422.1528 12.89CV 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 22.1528 2461152.6528 12.99 06:01:30.91 +44:57:14.5
167.61866 10.72290 galactic Aur Second-epoch detections are separated by 1.5" and 4.8 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 | 06:01:30.91 +44:57:14.5 (user input) | T | P | (position from user input) J-Ks=0.625+/-0.030 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:01:30.91 +44:57:14.5: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:01:30.91 +44:57:14.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,12.99,0.05,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 20260422.1528 12.99CV 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 22.1528 2461152.6528 13.05 05:57:12.00 +42:33:33.5
169.38192 8.90000 galactic Aur Second-epoch detections are separated by 2.9" and 5.1 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 | 05:57:12.00 +42:33:33.5 (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 05:57:12.00 +42:33:33.5: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:57:12.00 +42:33:33.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 13.05CV 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 22.1528 2461152.6528 13.12 05:48:07.96 +49:40:40.2
162.29114 10.98723 galactic Aur Second-epoch detections are separated by 4.8" and 4.8 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 211466700549060736 | 05:48:06.23 +49:40:13.7 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.562+/-0.030 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:48:07.96 +49:40:40.2: 14.75 +/- 0.31 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:48:07.96 +49:40:40.2: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211466700549060736,2461152.6528,13.12,0.05,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 211466700549060736 20260422.1528 13.12CV 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 22.1528 2461152.6528 12.98 05:43:22.58 +48:15:22.5
163.15041 9.60326 galactic Aur Second-epoch detections are separated by 2.8" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.8484+48.2557 | 05:43:22.58 +48:15:22.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:43:22.58 +48:15:22.5: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:43:22.58 +48:15:22.5: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 J085.8484+48.2557,2461152.6528,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.8484+48.2557 20260422.1528 12.98CV 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 22.1528 2461152.6528 13.12 06:23:09.77 +49:09:60.0
165.35432 15.86619 galactic Aur Second-epoch detections are separated by 0.2" and 4.8 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 | 06:23:09.77 +49:09:60.0 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.349+/-0.036 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:23:09.77 +49:09:60.0: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:23:09.77 +49:09:60.0: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,13.12,0.05,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 20260422.1528 13.12CV 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 22.1528 2461152.6528 13.05 06:01:16.82 +47:35:44.4
165.21223 11.91128 galactic Aur Second-epoch detections are separated by 1.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.3023+47.5982 | 06:01:16.82 +47:35:44.4 (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 06:01:16.82 +47:35:44.4: 14.89 +/- 0.35 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:01:16.82 +47:35:44.4: 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+47.5982,2461152.6528,13.05,0.05,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 J090.3023+47.5982 20260422.1528 13.05CV 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 22.1528 2461152.6528 13.17 06:23:05.38 +49:11:47.2
165.32097 15.86701 galactic Aur Second-epoch detections are separated by 4.1" and 5.0 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 J095.7693+49.1987 | 06:23:05.38 +49:11:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.284+/-0.040 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:23:05.38 +49:11:47.2: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:23:05.38 +49:11:47.2: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.7693+49.1987,2461152.6528,13.17,0.05,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 J095.7693+49.1987 20260422.1528 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1528 2461152.6528 13.10 05:37:41.43 +45:58:09.2
164.63027 7.59702 galactic Aur Second-epoch detections are separated by 0.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J053745.20+455814.5 | 05:37:45.20 +45:58:14.5 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.501+/-0.038 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:37:41.43 +45:58:09.2: 14.47 +/- 0.24 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:37:41.43 +45:58:09.2: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053745.20+455814.5,2461152.6528,13.10,0.05,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
ASASSN-V J053745.20+455814.5 20260422.1528 13.10CV 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 22.1528 2461152.6528 13.23 06:04:15.61 +46:54:36.2
166.07189 12.04751 galactic Aur Second-epoch detections are separated by 1.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.0747+46.9169 | 06:04:15.61 +46:54:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.482+/-0.034 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:04:15.61 +46:54:36.2: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:04:15.61 +46:54:36.2: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.0747+46.9169,2461152.6528,13.23,0.05,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 J091.0747+46.9169 20260422.1528 13.23CV 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 22.1528 2461152.6528 13.16 06:17:09.55 +47:00:39.6
166.96714 14.07062 galactic Aur Second-epoch detections are separated by 1.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:17:09.55 +47:00:39.6 (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 06:17:09.55 +47:00:39.6: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:17:09.55 +47:00:39.6: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 13.16CV 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 22.1528 2461152.6528 13.06 05:37:52.51 +43:02:34.8
167.15440 6.08593 galactic Aur Second-epoch detections are separated by 0.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:37:52.51 +43:02:34.8 (user input) | T | P | (position from user input) J-Ks=1.389+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:37:52.51 +43:02:34.8: 13.47 +/- 0.11 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:37:52.51 +43:02:34.8: 14.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6528,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1528 13.06CV 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 22.1528 2461152.6528 13.42 06:09:50.60 +49:17:44.2
164.30132 13.94039 galactic Aur Second-epoch detections are separated by 2.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.4504+49.2934 | 06:09:47.14 +49:17:12.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:09:50.60 +49:17:44.2: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:09:50.60 +49:17:44.2: 14.28 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.4504+49.2934,2461152.6528,13.42,0.05,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
ATO J092.4504+49.2934 20260422.1528 13.42CV 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 22.1528 2461152.6528 13.30 06:07:54.21 +45:58:47.0
167.21065 12.18801 galactic Aur Second-epoch detections are separated by 1.8" and 4.8 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 963318524057490944 | 06:07:52.35 +45:58:14.7 (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 06:07:54.21 +45:58:47.0: 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 06:07:54.21 +45:58:47.0: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963318524057490944,2461152.6528,13.30,0.05,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 963318524057490944 20260422.1528 13.30CV 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 22.1528 2461152.6528 13.37 06:10:00.20 +45:32:42.1
167.77590 12.32205 galactic Aur Second-epoch detections are separated by 0.4" and 4.8 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 963235824465355264 | 06:09:58.38 +45:33:23.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.036 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:10:00.20 +45:32:42.1: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:10:00.20 +45:32:42.1: 14.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963235824465355264,2461152.6528,13.37,0.05,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 963235824465355264 20260422.1528 13.37CV 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 22.1528 2461152.6528 13.31 05:56:58.10 +46:41:29.6
165.67852 10.84077 galactic Aur Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.2314+46.6988 | 05:56:58.10 +46:41:29.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.034 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:56:58.10 +46:41:29.6: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:56:58.10 +46:41:29.6: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2314+46.6988,2461152.6528,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2314+46.6988 20260422.1528 13.31CV 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 22.1528 2461152.6528 13.57 06:17:28.87 +48:00:53.8
166.04953 14.53995 galactic Aur Second-epoch detections are separated by 2.6" and 4.9 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 969171572345044352 | 06:17:24.79 +48:01:10.7 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.375+/-0.045 (G)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:17:28.87 +48:00:53.8: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:17:28.87 +48:00:53.8: 14.59 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 969171572345044352,2461152.6528,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 969171572345044352 20260422.1528 13.57CV 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 22.1528 2461152.6528 13.38 06:10:45.19 +48:16:56.3
165.30883 13.63734 galactic Aur Second-epoch detections are separated by 2.7" and 4.8 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 J092.6873+48.2843 | 06:10:45.19 +48:16:56.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.222+/-0.035 (F)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 06:10:45.19 +48:16:56.3: 13.90 +/- 0.12 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:10:45.19 +48:16:56.3: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6873+48.2843,2461152.6528,13.38,0.05,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 J092.6873+48.2843 20260422.1528 13.38CV 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 22.1528 2461152.6528 13.57 05:47:45.82 +45:04:51.1
166.31370 8.65733 galactic Aur Second-epoch detections are separated by 1.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.9565+45.0681 | 05:47:47.14 +45:04:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.528+/-0.033 (K)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits at 05:47:45.82 +45:04:51.1: 14.58 +/- 0.23 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:47:45.82 +45:04:51.1: 14.58 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.9565+45.0681,2461152.6528,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.9565+45.0681 20260422.1528 13.57CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461152.6528,11.31,0.05,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
VY Aur 20260422.1528 11.31CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461152.6528,10.34,0.05,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
AC Aur 20260422.1528 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
## 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: 2461152.65309660 22.04.2026 03:40:17.546 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
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: 8 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): 22845
Objects passed selection criteria: 22799
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 19080.2
Average stars matched: 18652.8 (97.7595 %)
Memory usage VmPeak: 126880 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 Tue Apr 21 22:50:20 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: 2461152.65309660 22.04.2026 03:40:17.546 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 346
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: 112 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): 158501
Objects passed selection criteria: 158197
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 142697
Average stars matched: 138498 (97.0571 %)
Memory usage VmPeak: 1982076 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 Tue Apr 21 22:55:19 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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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: 2461152.65240898
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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Image size: 941.5'x626.6' 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: 06:00:12.355 +45:59:33.13 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 06:00:12.355 +45:59:33.13
Angular distance between the image centers 0.0731 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
Image size: 941.5'x626.6' 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: 06:00:11.274 +45:59:07.89 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 06:00:11.274 +45:59:07.89
Angular distance between the image centers 0.0721 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 06:00:12.355 +45:59:33.13
Second-epoch second image center 06:00:11.274 +45:59:07.89
Angular distance between the image centers 0.00768 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.CnbjjMpkpQ
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.WYBPsYnZce
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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits &> /tmp/tmp.bu4eU5sLLa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits &> /tmp/tmp.aU8AWadtIN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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 10 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
2.2 pix fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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
14.8 mag. fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
14.8 mag. fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.CnbjjMpkpQ (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/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.WYBPsYnZce (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/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.bu4eU5sLLa (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1015, passed=14176
Got 14176 stars (including 13137 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat
util/solve_plate_with_UCAC5 got 14176 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 936 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(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 13894 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 936 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(), 13893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 13893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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.aU8AWadtIN (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=973, passed=14075
Got 14075 stars (including 13083 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat
util/solve_plate_with_UCAC5 got 14075 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31670.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31503_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31503_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:17:54.69 +41:11:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 2.024 195065736570175232 079.47860479966 +41.19823177411 10.9555 10.7152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31541_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31541_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:14:59.12 +46:47:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31542_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31542_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:34:27.52 +44:52:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)GAIADR2_OUTPUT=# 0.520 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31564_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31564_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:59:43.45 +44:59:09.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31583_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31583_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:37:23.04 +46:49:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 0.783 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31632_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31632_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:45:42.91 +43:37:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31670_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 31670_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:46:04.83 +47:26:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.422 966672004459585152 101.51999576409 +47.43461621313 12.0973 11.3733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:41:12.82 +44:09:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 02325_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:27:04.77 +50:07:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:26:01.82 +50:29:27.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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 ####
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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Image size: 941.5'x626.6' 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: 06:00:12.355 +45:59:33.13 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 06:00:12.355 +45:59:33.13
Angular distance between the image centers 0.0731 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
Image size: 941.5'x626.6' 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: 06:00:11.274 +45:59:07.89 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 06:00:11.274 +45:59:07.89
Angular distance between the image centers 0.0721 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 06:00:12.355 +45:59:33.13
Second-epoch second image center 06:00:11.274 +45:59:07.89
Angular distance between the image centers 0.00768 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.GoE56FN4wx
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.HbRCi40zfr
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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits &> /tmp/tmp.ySaPlYZByC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits &> /tmp/tmp.F4zLXgTx0x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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 336 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
2.1 pix fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
2.1 pix fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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
13.9 mag. fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
13.9 mag. fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.GoE56FN4wx (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/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.HbRCi40zfr (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/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.ySaPlYZByC (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=8034, passed=116487
Got 116487 stars (including 108255 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat
util/solve_plate_with_UCAC5 got 116487 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 39.8 to 51.4)
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(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 114118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 39.8 to 51.4)
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(), 114120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 114120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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.F4zLXgTx0x (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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=7931, passed=116558
Got 116558 stars (including 108438 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat
util/solve_plate_with_UCAC5 got 116558 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 39.8 to 51.4)
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: 932 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 114117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 39.8 to 51.4)
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: 932 matched stars entering correct_measured_positions(), 114115 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 114115 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-39-18_20.00sec_-4.90C_LIGHTs_0059.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.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_2026-04-21_CI_Aur-02-Q1b1x1_224117_TTUQ1b1x1_3811536_3Qa2YFGi/wcs_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out15085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196915.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): 166s
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: 40s
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Considering the candidate 195181_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195181_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195190_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195190_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:52:15.74 +45:47:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.944 197651169443704448 088.06544000779 +45.79052007687 14.2561 13.4931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195202_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195202_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:14:05.67 +46:10:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 0.351 962623637006130048 093.52369081465 +46.16944738936 14.4186 13.8943 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 195204_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195204_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:01:01.95 +48:38:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.523 969814580490083584 090.25833473206 +48.64796014011 14.3056 13.6622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195205_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:59.39 +49:26:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.246 211286694176443648 089.24755543055 +49.44861273434 14.4035 13.8229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195219_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195219_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:09.18 +45:22:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.789 196739021469243136 089.28834194525 +45.38023735729 13.9714 13.3170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195238_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195238_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195241_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195241_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:44:36.85 +46:43:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.795 209668384859666048 086.15384962110 +46.72668476459 13.9845 13.4608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195245_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195245_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:47:50.33 +43:23:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.305 196094638936759168 086.96020415910 +43.39040464429 14.0631 13.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195246_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195246_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:05:39.31 +42:41:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195252_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195252_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:14:15.75 +47:53:18.8: 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 06:14:15.75 +47:53:18.8: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.06
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Considering the candidate 195261_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195261_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:37:43.78 +50:23:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195268_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195268_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:49.09 +47:17:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.423 211950180726200960 080.45553127216 +47.28875661514 13.9802 13.3201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195272_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195272_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:20:27.53 +46:35:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195277_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195277_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195280_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195280_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:24:03.22 +44:40:41.0: 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 06:24:03.22 +44:40:41.0: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
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Considering the candidate 195283_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195283_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:36:25.37 +41:59:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195284_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195284_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195287_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195287_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 195289_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195289_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:29.58 +45:53:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.878 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195290_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195290_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:25:18.49 +47:51:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195291_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195291_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:35:51.39 +48:37:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.782 967736537873159552 098.96442617276 +48.62908682184 13.9840 13.4169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195293_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195293_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:33:19.95 +49:59:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195294_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195294_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:22:50.64 +41:27:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195295_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195295_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:08:44.10 +48:20:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195296_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:33.89 +45:13:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195301_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195301_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:53.94 +47:59:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195302_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195302_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:18:32.74 +46:16:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.735 211837721303196800 079.63671201134 +46.28305578216 13.5567 13.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195307_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195307_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:27:16.27 +45:33:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.211 208891717333926528 081.81826265908 +45.55967745585 13.5125 13.0409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195310_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195310_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:22:59.55 +44:37:30.9: 12.92 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:22:59.55 +44:37:30.9: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.04
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Considering the candidate 195312_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195312_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:31:27.67 +47:36:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195313_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:23:24.91 +46:08:34.8: 12.16 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:23:24.91 +46:08:34.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
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Considering the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195316_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195316_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:33:14.94 +46:13:28.6: 12.77 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:33:14.94 +46:13:28.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
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Considering the candidate 195323_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195323_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:43:44.29 +50:59:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.408 215225007387998592 085.93446186108 +50.98390711228 13.5660 12.9195 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 195324_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195324_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:32:53.72 +50:04:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195329_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195329_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:16:43.95 +44:42:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.239 962379987803965824 094.18319043390 +44.71153534768 13.5579 13.0286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195330_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195330_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:31.11 +47:10:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.283 209270842686354944 082.12954725612 +47.18122494840 13.2241 12.2315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195331_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:32:05.46 +45:22:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195333_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195333_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:19:47.24 +42:06:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195334_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195334_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:42:17.97 +47:48:57.0 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 195335_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195335_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:16:36.25 +44:32:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.654 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195337_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195337_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:11:13.13 +47:02:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.100 969416385483084800 092.80474694837 +47.04423121691 13.2454 12.7727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195338_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195338_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:22.97 +46:50:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195339_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195339_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:42:01.71 +46:28:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.670 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195346_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195346_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:00.16 +43:23:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195347_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195347_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:31:36.48 +45:36:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195348_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195348_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:39:24.10 +41:20:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195349_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:19:24.74 +42:28:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195350_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195350_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:47:05.76 +48:25:26.5: 13.90 +/- 0.16 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:47:05.76 +48:25:26.5: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
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Considering the candidate 195354_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195354_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:25:35.51 +49:58:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195357_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195357_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:47.67 +43:12:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195358_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195358_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:20:12.78 +43:38:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.162 961773920675999104 095.05336462401 +43.64875630381 12.9196 12.2182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195361_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195361_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:40:23.58 +49:53:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195362_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195362_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:51:38.16 +48:20:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.187 210370418736729472 087.90946632657 +48.33580450234 12.7164 12.1774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195364_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195364_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:35:28.87 +47:01:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.894 210567300037906816 083.87064439310 +47.03086736119 12.1803 11.3066 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 195367_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195367_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:46.01 +43:34:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195369_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195369_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:57:09.02 +46:13:43.3: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:57:09.02 +46:13:43.3: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
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Considering the candidate 195371_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195371_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:56:09.57 +44:17:59.5: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:56:09.57 +44:17:59.5: 11.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
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Considering the candidate 195373_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195373_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:17:54.66 +41:11:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.07, MAG_FAINT_SEARCH_LIMIT=11.05)GAIADR2_OUTPUT=# 2.852 195065736570175232 079.47860479966 +41.19823177411 10.9555 10.7152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195440_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195440_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:43:27.56 +42:19:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.14, MAG_FAINT_SEARCH_LIMIT=11.12)GAIADR2_OUTPUT=# 0.438 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195444_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195444_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:44:52.57 +49:21:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195457_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:37:22.97 +46:49:18.5: 14.04 +/- 0.19 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:37:22.97 +46:49:18.5: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
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Considering the candidate 195512_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195512_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195549_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195549_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:05:46.61 +48:14:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195552_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195552_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:11:34.56 +48:44:35.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195564_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195564_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:31:20.53 +46:01:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195585_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195585_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:25:37.68 +45:40:57.1: 11.67 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:25:37.68 +45:40:57.1: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
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Considering the candidate 195596_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195596_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:26:48.03 +43:44:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195610_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195610_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:43:31.45 +50:41:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.671 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195615_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195615_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:04:44.13 +46:34:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 0.394 963538701262091904 091.18394519730 +46.58109813512 12.4714 12.0753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195628_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195628_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:19:04.22 +47:21:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.280 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195635_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195635_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195639_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195639_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:19:01.51 +41:06:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195655_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195655_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:36:59.29 +48:07:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.028 967332673508208256 099.24717563820 +48.11763216666 12.6763 12.2075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195661_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195661_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:06:21.38 +48:46:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.260 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195679_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195679_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:33:38.42 +45:26:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195707_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195707_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195714_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195714_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:13:46.68 +44:43:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.492 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195716_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195716_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:15:03.58 +48:49:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.724 969337323724612608 093.76493977175 +48.82277166858 12.8238 12.2993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195724_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195724_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195727_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195727_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195733_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195733_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:18:49.01 +44:36:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195754_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195754_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195760_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195760_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195762_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195762_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:39:07.56 +44:53:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.236 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195767_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195767_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:29:20.87 +45:46:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195769_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195769_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195774_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195774_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:05:50.22 +44:39:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.563 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195781_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195781_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:18:23.45 +48:55:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195789_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195789_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:44:20.17 +47:42:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195793_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195793_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:34:37.52 +45:55:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195797_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195797_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195803_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195803_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:32:51.84 +42:57:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195818_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195818_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:40.90 +44:01:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.833 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195824_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195824_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:08.54 +49:03:09.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195825_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195825_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:09.66 +47:19:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.331 212316245079377280 081.04053074053 +47.31751152611 12.7573 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195831_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195831_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:26:51.32 +41:14:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 1.405 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195835_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195835_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:48:46.03 +46:35:01.7: 13.49 +/- 0.09 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:48:46.03 +46:35:01.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
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Considering the candidate 195841_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195841_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:02.44 +49:49:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.424 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 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 195846_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195846_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195864_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195864_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:40:42.94 +48:20:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.271 210971336200363648 085.17944784055 +48.33622155749 13.2097 12.6468 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 195866_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195866_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:22:39.81 +47:54:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.249 212586660519063680 080.66597215012 +47.91400751652 13.0455 12.2084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195873_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195873_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:11.11 +43:58:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195874_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195874_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:46.10 +45:53:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.672 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195885_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195885_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:17:28.77 +45:52:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.252 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195886_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195886_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:30:40.68 +41:28:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195890_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195890_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:43.93 +41:18:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.595 194505771619147776 082.18314538158 +41.30272918703 13.1352 12.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195894_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195894_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:45:59.78 +41:14:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.283 192676360365419264 086.49878011806 +41.24863519669 13.0621 12.1850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195896_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195896_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:03:13.59 +42:56:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195898_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195898_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:12:10.18 +50:14:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195900_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195900_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:59:52.73 +44:00:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.486 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195907_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195907_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:11:06.02 +41:55:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.060 960956566924526336 092.77506168430 +41.93017064148 13.2400 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195908_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195908_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:41:16.76 +47:26:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.575 210685257018537344 085.32032670455 +47.44841135014 13.1638 12.3736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195909_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195909_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:44.66 +46:30:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195911_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195911_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:17:56.68 +46:08:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195923_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195923_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:00.95 +44:14:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.475 193599537815354240 089.00397047386 +44.24771493026 13.3067 12.4824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195934_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195934_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 195935_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195935_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:13:42.22 +45:31:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195937_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195937_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:32.60 +43:42:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.693 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 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 195942_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195942_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:01:32.42 +47:32:25.6: 11.75 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:01:32.42 +47:32:25.6: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
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Considering the candidate 195950_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195950_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:53:12.08 +45:24:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.043 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195953_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195953_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:15:42.76 +42:02:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195958_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195958_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:35:17.74 +42:18:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195959_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195959_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:52.01 +41:16:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.687 194180797215485440 081.21738962468 +41.28187659990 12.4521 11.0529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195974_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195974_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:11:01.06 +47:29:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.207 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195979_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195979_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:03:22.92 +42:40:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195990_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195990_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:32:56.53 +48:00:33.5: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:32:56.53 +48:00:33.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
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Considering the candidate 195992_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195992_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:30:53.86 +49:47:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195993_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195993_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:18:48.26 +44:06:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.243 207680158599604608 079.70193351269 +44.11312538601 13.3106 12.6161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195996_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 195996_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:40:14.25 +50:00:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195997_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 195997_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196001_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196001_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196006_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196006_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:11:49.27 +45:03:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196009_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196009_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:17:34.83 +46:23:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196015_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196015_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:17.27 +43:16:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196023_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196023_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:01:04.66 +50:00:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.451 970368734350565760 090.26951411061 +50.00316418749 13.2862 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196025_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196025_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:53:06.81 +44:55:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.363 196796780189493888 088.27871551763 +44.93359735580 13.4264 12.8611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196033_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196033_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:47:45.33 +50:03:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.573 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196036_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196036_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:40:25.85 +48:47:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196047_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196047_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:19:23.12 +42:09:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196049_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196049_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:01.34 +48:14:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.222 212655861031529216 082.00598407831 +48.25025093485 13.3563 12.8993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196054_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196054_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:56:51.35 +48:55:52.7: 12.39 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:56:51.35 +48:55:52.7: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
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Considering the candidate 196057_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196057_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:30:57.13 +43:05:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196059_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:17:09.41 +43:26:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196060_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196060_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:08:02.34 +46:40:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 0.645 963435214026488704 092.00979468381 +46.68289863325 13.5967 13.1319 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 196062_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196062_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:13:22.45 +44:28:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196070_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196070_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:52:03.68 +49:32:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196075_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196075_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:26:06.67 +46:10:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196089_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196089_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:06.21 +45:12:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196091_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196091_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:29:04.62 +42:17:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196092_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196092_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:07:30.01 +46:55:56.5: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:07:30.01 +46:55:56.5: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
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Considering the candidate 196098_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196098_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:04:07.18 +41:10:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196100_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196100_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:30:09.28 +46:12:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.183 209019462542689408 082.53951456145 +46.21579217952 13.5370 12.9587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196108_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196108_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196112_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196112_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:27:50.44 +42:19:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196117_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196117_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:22:46.50 +47:55:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196118_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196118_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:28:50.32 +49:26:29.3: 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 05:28:50.32 +49:26:29.3: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
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Considering the candidate 196126_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196126_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:33:56.62 +46:11:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.135 208282721033602560 083.48553101272 +46.19874907056 13.4787 12.6535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196129_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196129_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:44.81 +44:40:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.509 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196132_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196132_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:38:27.31 +41:13:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.575 191329557403012096 084.61349900374 +41.23148611486 13.6414 12.8401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196142_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196142_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196143_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196143_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:20.52 +42:46:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196144_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196144_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:12:03.06 +41:43:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.438 960200034204636544 093.01317175941 +41.73174612260 13.5765 12.8505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196147_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196147_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:22:30.65 +46:12:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.189 968436170866744448 095.62879686623 +46.20538276046 13.7294 12.9970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196148_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196148_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:10:07.73 +42:07:48.8: 13.24 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:10:07.73 +42:07:48.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
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Considering the candidate 196149_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196149_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:54:46.98 +46:08:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.458 197756344602976384 088.69592668878 +46.14675681897 13.1311 12.0714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196151_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196151_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:17:15.71 +41:56:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.755 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196154_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196154_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:43:06.53 +44:51:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.277 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196156_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196156_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196160_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196160_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:30.92 +46:14:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.192 197751809117411712 089.12908358575 +46.24714326154 13.6175 12.8385 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 196161_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196161_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:38:22.05 +42:59:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.010 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196166_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196166_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:38:38.18 +41:51:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196167_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196167_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:38:46.55 +46:04:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.774 209541769223400064 084.69366740623 +46.06689801652 13.5146 12.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196168_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196168_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196171_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196171_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:35:09.59 +47:24:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.845 967208497413814656 098.79023955351 +47.41413739365 13.7156 13.0138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196172_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196172_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:34:02.57 +46:44:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196175_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196175_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:50.61 +44:16:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196181_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196181_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:41.22 +48:21:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196182_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196182_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196186_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196186_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:16:35.98 +45:44:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196187_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196187_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:25:57.51 +43:06:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.182 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196189_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196189_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:53:17.94 +43:17:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196194_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196194_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:25:45.47 +45:22:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196196_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196196_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:18:25.42 +48:30:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196198_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196198_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:49.28 +49:49:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196200_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196200_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:23:23.63 +50:13:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.354 261808836861057408 080.84799330687 +50.23144343721 13.3252 12.3513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196203_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196203_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:38.58 +41:49:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196208_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196208_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:35:35.21 +44:15:15.6: 12.68 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:35:35.21 +44:15:15.6: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
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Considering the candidate 196209_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196209_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196211_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196211_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:37:28.45 +42:00:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196213_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196213_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:31:01.84 +44:18:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196218_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196218_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196222_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196222_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:57:46.83 +43:35:11.8: 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 05:57:46.83 +43:35:11.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
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Considering the candidate 196226_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196226_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196231_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196231_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:22:01.85 +42:43:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 0.208 195300447945544064 080.50775878561 +42.71881683081 13.4492 12.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196238_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196238_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196240_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196240_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:41.57 +50:41:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.125 261875155450928384 080.42251070654 +50.69932540948 13.4670 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196243_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196243_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:32:30.32 +41:38:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196245_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196245_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:23:54.13 +46:06:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196246_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196246_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:34:32.04 +41:33:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196250_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196250_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196253_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196253_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:00:14.04 +47:43:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.859 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196254_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196254_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:42:29.87 +44:44:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.250 197245582797409152 085.62447289270 +44.74687417395 12.5370 11.1711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196255_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196255_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196259_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196259_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:20:02.75 +46:37:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196264_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196264_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:48:23.24 +49:46:58.0: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:48:23.24 +49:46:58.0: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
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Considering the candidate 196266_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196266_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:22:17.39 +46:57:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.698 211927228421172992 080.57195142662 +46.96253291072 13.6003 12.8490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196269_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196269_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:59:38.10 +42:04:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.110 192175086142767488 089.90835088276 +42.07327983836 13.8061 12.9402 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 196270_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196270_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:31.29 +47:51:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.864 210289196612409472 087.38044179706 +47.86209697171 13.6067 12.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196274_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196274_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196276_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196276_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:32:56.26 +48:45:34.9: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:32:56.26 +48:45:34.9: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
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Considering the candidate 196280_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196280_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:31:00.35 +42:54:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196281_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196281_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:34:02.84 +49:04:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196288_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196288_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:31:40.37 +42:51:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196289_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196289_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:24:21.78 +47:52:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196298_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196298_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:02:52.42 +45:42:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.855 963146592224643200 090.71840891408 +45.70231821898 13.6956 12.9106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196303_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196303_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:43:56.69 +47:43:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.128 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196309_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196309_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:47:21.09 +48:12:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196315_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196315_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:28:41.27 +48:14:36.2: 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 05:28:41.27 +48:14:36.2: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
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Considering the candidate 196320_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196320_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:33.81 +45:29:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196321_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196321_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:38:50.43 +49:49:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196323_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196323_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:44:39.81 +43:57:55.5: 12.51 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:44:39.81 +43:57:55.5: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
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Considering the candidate 196324_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196324_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:38:36.22 +49:43:23.2: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:38:36.22 +49:43:23.2: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
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Considering the candidate 196326_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196326_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:59:59.09 +43:51:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196327_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196327_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:33:21.98 +43:06:48.5: 12.25 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:33:21.98 +43:06:48.5: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.03
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Considering the candidate 196329_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196329_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:01:37.16 +46:50:34.4: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:01:37.16 +46:50:34.4: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
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Considering the candidate 196330_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196330_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196331_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196331_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:20:37.00 +49:04:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196332_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196332_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:37:40.62 +43:34:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.258 197035168055591296 084.42000576759 +43.57902834396 13.6158 12.9805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196342_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196342_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:46:39.83 +43:21:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196344_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196344_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:58:13.64 +42:51:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.398 192497895884100864 089.55761517572 +42.85400624846 13.8079 13.3003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196345_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196345_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:37:16.28 +44:02:48.8: 12.87 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:37:16.28 +44:02:48.8: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.04
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Considering the candidate 196358_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196358_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:27:03.66 +46:04:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196361_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196361_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:24.88 +49:14:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196363_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196363_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:25:29.24 +49:47:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196367_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196367_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196372_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196372_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:37:19.55 +44:51:37.6: 13.22 +/- 0.07 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:37:19.55 +44:51:37.6: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
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Considering the candidate 196385_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196385_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:40:59.60 +46:21:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.839 209552042785104768 085.24823356916 +46.36291720392 13.8385 13.1940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196389_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196389_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:08:04.95 +45:02:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.698 962871027122871040 092.02043346573 +45.03427793519 13.9306 13.3249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196392_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196392_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:40.86 +41:24:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196397_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196397_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196398_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196398_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:33:32.12 +48:16:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196402_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196402_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:51:18.87 +43:17:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.564 193427528667708288 087.82879815788 +43.29576806055 13.9092 13.2559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196407_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196407_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:03:21.16 +42:41:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196409_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196409_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:27.88 +47:51:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196414_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196414_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:39:32.64 +41:57:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196416_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196416_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:45.38 +45:54:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.595 196999777523639936 089.43970142505 +45.91480103623 13.9429 13.4194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196421_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196421_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:13:33.64 +48:03:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.732 969210708089081216 093.39001337563 +48.05522019758 14.0114 13.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196422_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196422_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:26:28.33 +42:41:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196430_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196430_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:28:45.84 +49:11:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196448_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196448_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196451_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196451_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:53:28.89 +46:52:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.630 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196461_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196461_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:52:21.17 +42:50:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196472_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196472_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:12:20.05 +50:12:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.754 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196474_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196474_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:53.27 +46:05:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.885 197005378160950784 089.47179707530 +46.09439219961 14.0011 13.1854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196478_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196478_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:03:18.86 +42:41:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196479_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196479_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:30:25.98 +49:51:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196484_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196484_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:47:49.09 +51:04:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196489_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196489_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:52:59.24 +46:57:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196495_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196495_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196497_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196497_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:25:56.84 +45:50:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.346 208940439442504192 081.48732215526 +45.84979359311 13.8726 13.2973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196505_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196505_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196506_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196506_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:53:51.92 +50:42:48.8: 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 05:53:51.92 +50:42:48.8: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.06
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Considering the candidate 196508_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196508_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196515_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196515_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:28:18.27 +44:16:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.815 207789005953568000 082.07681950966 +44.26697163248 13.7769 12.9413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196516_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196516_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:35:41.30 +44:16:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196522_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196522_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:39:00.00 +47:35:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.629 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196523_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196523_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196527_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196527_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196533_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196533_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:52:55.05 +42:18:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196534_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196534_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:04:26.11 +44:42:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.889 962954486927751680 091.10989751367 +44.70182838307 14.1586 13.5091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196536_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196536_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:26:13.36 +46:47:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196537_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196537_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196544_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196544_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:42:50.68 +48:07:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.248 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 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 196548_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196548_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:48:07.75 +50:26:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.232 214568598946171264 087.03234717596 +50.43577947810 13.9372 13.3806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196551_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196551_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:26:29.91 +49:54:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 0.380 971091731965538688 096.62459838265 +49.90271527912 14.1099 13.5701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196554_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196554_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:23:01.84 +46:43:26.9: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:23:01.84 +46:43:26.9: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
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Considering the candidate 196560_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196560_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 196563_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196563_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:40:34.21 +46:53:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196571_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196571_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:03:43.65 +50:12:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196579_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196579_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:46:32.89 +45:16:05.1: 11.34 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:46:32.89 +45:16:05.1: 14.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
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Considering the candidate 196587_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196587_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196593_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196593_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196596_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196596_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:53:58.69 +46:09:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196597_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196597_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:19:05.46 +46:34:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196605_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196605_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:29:32.33 +48:50:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 0.988 212734441750616576 082.38435419683 +48.83832739506 14.0076 13.1565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196619_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196619_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:17:15.26 +42:06:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196623_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196623_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:31:19.99 +45:58:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.443 208252729279086464 082.83335404737 +45.97527379616 13.9254 13.0817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196624_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196624_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:41:07.33 +47:58:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196634_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196634_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:13:29.98 +47:17:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.790 968785712485462016 093.37489471116 +47.29624681696 14.0869 13.4852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196640_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196640_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:36:18.66 +47:12:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.620 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196660_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196660_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196661_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196661_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:41.64 +49:06:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196663_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196663_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196664_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196664_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:34:15.75 +44:17:05.2: 12.86 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:34:15.75 +44:17:05.2: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
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Considering the candidate 196665_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196665_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:49:25.45 +42:20:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.341 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196669_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196669_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:48:44.65 +49:34:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.705 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 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 196670_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196670_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:11.33 +42:50:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.693 192511364902195840 089.29695470380 +42.84027162771 14.0339 13.4622 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 196672_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196672_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:34:19.15 +44:27:43.7: 13.02 +/- 0.06 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:34:19.15 +44:27:43.7: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
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Considering the candidate 196674_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196674_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:56:00.73 +49:05:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.306 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196675_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196675_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:36:36.48 +40:24:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.903 957264857849652096 099.15186376391 +40.41364502642 14.3409 13.8338 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 196680_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196680_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196683_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196683_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196704_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196704_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196719_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196719_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:11:51.81 +45:03:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 0.911 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196721_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196721_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:00:37.81 +42:52:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.889 960918363191448960 090.15755383159 +42.86827457081 13.9851 13.4256 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#
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Considering the candidate 196735_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196735_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196760_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196760_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:50:06.43 +46:08:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196777_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196777_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:19:35.18 +50:11:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196784_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196784_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:39:33.80 +49:48:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.855 214254688376903680 084.89157910286 +49.80984354835 14.2849 13.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196788_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196788_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:36:17.25 +47:13:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196789_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196789_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 05:49:15.68 +45:41:15.6: 14.84 +/- 0.32 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 05:49:15.68 +45:41:15.6: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
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Considering the candidate 196790_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196790_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:32:56.40 +50:48:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.942 215347568575186688 083.23502356000 +50.80367783911 13.8986 12.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196800_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196800_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 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 06:09:37.23 +50:22:55.1: 12.74 +/- 0.05 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits at 06:09:37.23 +50:22:55.1: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
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Considering the candidate 196801_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196801_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:47:10.95 +46:03:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.391 197523351216767360 086.79557643499 +46.05504755708 14.1430 13.2999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196806_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196806_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:17.25 +47:02:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196807_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196807_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:10:13.60 +49:41:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 0.471 970161854365804544 092.55679867882 +49.68720630293 14.1192 13.2925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196813_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196813_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:45:03.94 +49:39:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.397 214110446194930560 086.26624730253 +49.65684395412 14.4453 13.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196828_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196828_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
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Considering the candidate 196859_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196859_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:58:09.63 +48:37:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.097 210251469618523520 089.54055114472 +48.62003298825 14.3909 13.8430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196876_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196876_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:42:47.65 +45:58:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196893_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196893_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:03:02.80 +46:43:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.190 963597151473005312 090.76167548963 +46.73289191284 14.4883 13.8730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196915_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 196915_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196927_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196927_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:55:13.96 +46:35:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.204 197827297462305408 088.80839057683 +46.59107115062 14.6408 13.9416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196930_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 196930_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:19:28.32 +45:31:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:14:59.11 +46:47:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:37:57.02 +44:40:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:41:12.82 +44:09:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:57:23.88 +48:22:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
Preparing report for the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:21:29.97 +43:44:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 06:26:01.79 +50:29:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-21_22-40-17_20.00sec_-4.90C_LIGHTs_0060 did not pass the final checks
**** FOUND 05:59:44.15 +47:37:00.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 213s
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 ####
05:27:04.80 +50:07:23.2
06:14:02.99 +50:52:47.6
05:45:51.93 +50:23:48.2
05:53:45.75 +44:06:44.9
05:46:42.28 +41:24:56.8
05:16:30.05 +50:58:24.5
05:28:04.06 +49:28:28.7
05:46:26.50 +47:55:01.2
05:49:29.01 +44:16:19.6
06:21:48.26 +46:46:31.0
05:29:45.61 +49:44:06.0
05:29:21.98 +51:11:31.1
05:25:48.82 +43:15:17.9
05:42:07.70 +50:04:31.5
05:40:02.66 +50:02:05.9
05:48:04.13 +43:19:50.6
06:26:19.86 +41:59:11.2
06:47:21.13 +48:12:02.0
05:38:51.13 +41:49:43.2
06:01:40.60 +44:57:46.8
05:38:24.43 +42:59:47.8
06:20:04.37 +46:37:59.6
05:27:26.07 +44:48:51.3
05:28:11.73 +43:27:55.0
06:25:49.04 +48:15:43.3
05:54:13.34 +47:53:38.5
05:20:50.94 +44:04:37.2
06:02:32.13 +48:11:24.3
06:12:44.90 +47:30:43.0
05:31:42.96 +44:43:23.8
05:30:45.55 +43:28:05.8
05:35:29.73 +45:58:09.6
05:35:43.50 +44:16:09.7
06:01:30.91 +44:57:14.5
05:57:12.00 +42:33:33.5
05:48:07.96 +49:40:40.2
05:43:22.58 +48:15:22.5
06:23:09.77 +49:09:60.0
06:01:16.82 +47:35:44.4
06:23:05.38 +49:11:47.2
05:37:41.43 +45:58:09.2
06:04:15.61 +46:54:36.2
06:17:09.55 +47:00:39.6
05:37:52.51 +43:02:34.8
06:09:50.60 +49:17:44.2
06:07:54.21 +45:58:47.0
06:10:00.20 +45:32:42.1
05:56:58.10 +46:41:29.6
06:17:28.87 +48:00:53.8
06:10:45.19 +48:16:56.3
05:47:45.82 +45:04:51.1
06:09:51.95 +46:34:27.7
########### 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 ####
06:14:02.99 +50:52:47.6
05:45:51.93 +50:23:48.2
05:53:45.75 +44:06:44.9
05:46:42.28 +41:24:56.8
05:16:30.05 +50:58:24.5
05:28:04.06 +49:28:28.7
05:46:26.50 +47:55:01.2
05:49:29.01 +44:16:19.6
06:21:48.26 +46:46:31.0
05:29:45.61 +49:44:06.0
05:29:21.98 +51:11:31.1
05:25:48.82 +43:15:17.9
05:42:07.70 +50:04:31.5
05:40:02.66 +50:02:05.9
05:48:04.13 +43:19:50.6
06:26:19.86 +41:59:11.2
06:47:21.13 +48:12:02.0
05:38:51.13 +41:49:43.2
06:01:40.60 +44:57:46.8
05:38:24.43 +42:59:47.8
06:20:04.37 +46:37:59.6
05:27:26.07 +44:48:51.3
05:28:11.73 +43:27:55.0
06:25:49.04 +48:15:43.3
05:54:13.34 +47:53:38.5
05:20:50.94 +44:04:37.2
06:02:32.13 +48:11:24.3
06:12:44.90 +47:30:43.0
05:31:42.96 +44:43:23.8
05:30:45.55 +43:28:05.8
05:35:29.73 +45:58:09.6
05:35:43.50 +44:16:09.7
06:01:30.91 +44:57:14.5
05:57:12.00 +42:33:33.5
05:48:07.96 +49:40:40.2
05:43:22.58 +48:15:22.5
06:23:09.77 +49:09:60.0
06:01:16.82 +47:35:44.4
06:23:05.38 +49:11:47.2
05:37:41.43 +45:58:09.2
06:04:15.61 +46:54:36.2
06:17:09.55 +47:00:39.6
05:37:52.51 +43:02:34.8
06:09:50.60 +49:17:44.2
06:07:54.21 +45:58:47.0
06:10:00.20 +45:32:42.1
05:56:58.10 +46:41:29.6
06:17:28.87 +48:00:53.8
06:10:45.19 +48:16:56.3
05:47:45.82 +45:04:51.1
06:09:51.95 +46:34:27.7
05:27:04.80 +50:07:23.2
###################################################################################
06:14:02.99 +50:52:47.6 -- not an asteroid (will add it to exclusion list)
05:45:51.93 +50:23:48.2 -- not an asteroid (will add it to exclusion list)
05:53:45.75 +44:06:44.9 -- not an asteroid (will add it to exclusion list)
05:46:42.28 +41:24:56.8 -- not an asteroid (will add it to exclusion list)
05:16:30.05 +50:58:24.5 -- not an asteroid (will add it to exclusion list)
05:28:04.06 +49:28:28.7 -- not an asteroid (will add it to exclusion list)
05:46:26.50 +47:55:01.2 -- not an asteroid (will add it to exclusion list)
05:49:29.01 +44:16:19.6 -- not an asteroid (will add it to exclusion list)
06:21:48.26 +46:46:31.0 -- not an asteroid (will add it to exclusion list)
05:29:45.61 +49:44:06.0 -- not an asteroid (will add it to exclusion list)
05:29:21.98 +51:11:31.1 -- not an asteroid (will add it to exclusion list)
05:25:48.82 +43:15:17.9 -- not an asteroid (will add it to exclusion list)
05:42:07.70 +50:04:31.5 -- not an asteroid (will add it to exclusion list)
05:40:02.66 +50:02:05.9 -- not an asteroid (will add it to exclusion list)
05:48:04.13 +43:19:50.6 -- not an asteroid (will add it to exclusion list)
06:26:19.86 +41:59:11.2 -- not an asteroid (will add it to exclusion list)
06:47:21.13 +48:12:02.0 -- not an asteroid (will add it to exclusion list)
05:38:51.13 +41:49:43.2 -- not an asteroid (will add it to exclusion list)
06:01:40.60 +44:57:46.8 -- not an asteroid (will add it to exclusion list)
05:38:24.43 +42:59:47.8 -- not an asteroid (will add it to exclusion list)
06:20:04.37 +46:37:59.6 -- not an asteroid (will add it to exclusion list)
05:27:26.07 +44:48:51.3 -- not an asteroid (will add it to exclusion list)
05:28:11.73 +43:27:55.0 -- not an asteroid (will add it to exclusion list)
06:25:49.04 +48:15:43.3 -- not an asteroid (will add it to exclusion list)
05:54:13.34 +47:53:38.5 -- not an asteroid (will add it to exclusion list)
05:20:50.94 +44:04:37.2 -- not an asteroid (will add it to exclusion list)
06:02:32.13 +48:11:24.3 -- not an asteroid (will add it to exclusion list)
06:12:44.90 +47:30:43.0 -- not an asteroid (will add it to exclusion list)
05:31:42.96 +44:43:23.8 -- not an asteroid (will add it to exclusion list)
05:30:45.55 +43:28:05.8 -- not an asteroid (will add it to exclusion list)
05:35:29.73 +45:58:09.6 -- not an asteroid (will add it to exclusion list)
05:35:43.50 +44:16:09.7 -- not an asteroid (will add it to exclusion list)
06:01:30.91 +44:57:14.5 -- not an asteroid (will add it to exclusion list)
05:57:12.00 +42:33:33.5 -- not an asteroid (will add it to exclusion list)
05:48:07.96 +49:40:40.2 -- not an asteroid (will add it to exclusion list)
05:43:22.58 +48:15:22.5 -- not an asteroid (will add it to exclusion list)
06:23:09.77 +49:09:60.0 -- not an asteroid (will add it to exclusion list)
06:01:16.82 +47:35:44.4 -- not an asteroid (will add it to exclusion list)
06:23:05.38 +49:11:47.2 -- not an asteroid (will add it to exclusion list)
05:37:41.43 +45:58:09.2 -- not an asteroid (will add it to exclusion list)
06:04:15.61 +46:54:36.2 -- not an asteroid (will add it to exclusion list)
06:17:09.55 +47:00:39.6 -- not an asteroid (will add it to exclusion list)
05:37:52.51 +43:02:34.8 -- not an asteroid (will add it to exclusion list)
06:09:50.60 +49:17:44.2 -- not an asteroid (will add it to exclusion list)
06:07:54.21 +45:58:47.0 -- not an asteroid (will add it to exclusion list)
06:10:00.20 +45:32:42.1 -- not an asteroid (will add it to exclusion list)
05:56:58.10 +46:41:29.6 -- not an asteroid (will add it to exclusion list)
06:17:28.87 +48:00:53.8 -- not an asteroid (will add it to exclusion list)
06:10:45.19 +48:16:56.3 -- not an asteroid (will add it to exclusion list)
05:47:45.82 +45:04:51.1 -- not an asteroid (will add it to exclusion list)
06:09:51.95 +46:34:27.7 -- not an asteroid (will add it to exclusion list)
05:27:04.80 +50:07:23.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:16:30.05 +50:58:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.94 +44:04:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:48.82 +43:15:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.80 +50:07:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.07 +44:48:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:04.06 +49:28:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.73 +43:27:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:21.98 +51:11:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:45.61 +49:44:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:45.55 +43:28:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:42.96 +44:43:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:29.73 +45:58:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:43.50 +44:16:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.43 +45:58:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.51 +43:02:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:24.43 +42:59:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:51.13 +41:49:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.66 +50:02:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:07.70 +50:04:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:22.58 +48:15:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:51.93 +50:23:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:26.50 +47:55:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:42.28 +41:24:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:45.82 +45:04:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.13 +43:19:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:07.96 +49:40:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:29.01 +44:16:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:45.75 +44:06:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:13.34 +47:53:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:58.10 +46:41:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.00 +42:33:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.82 +47:35:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:30.91 +44:57:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:40.60 +44:57:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.13 +48:11:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:15.61 +46:54:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:54.21 +45:58:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:50.60 +49:17:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:51.95 +46:34:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:00.20 +45:32:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:45.19 +48:16:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:44.90 +47:30:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:02.99 +50:52:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:09.55 +47:00:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:28.87 +48:00:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:04.37 +46:37:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:48.26 +46:46:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:05.38 +49:11:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:09.77 +49:09:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:49.04 +48:15:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.86 +41:59:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:21.13 +48:12:02.0 -- 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)
05:16:30.05 +50:58:24.5 -- not a known variable star
05:20:50.94 +44:04:37.2 -- not a known variable star
05:25:48.82 +43:15:17.9 -- a known variable star
05:27:04.80 +50:07:23.2 -- a known variable star
05:27:26.07 +44:48:51.3 -- not a known variable star
05:28:04.06 +49:28:28.7 -- not a known variable star
05:28:11.73 +43:27:55.0 -- not a known variable star
05:29:21.98 +51:11:31.1 -- not a known variable star
05:29:45.61 +49:44:06.0 -- not a known variable star
05:30:45.55 +43:28:05.8 -- not a known variable star
05:31:42.96 +44:43:23.8 -- not a known variable star
05:35:29.73 +45:58:09.6 -- not a known variable star
05:35:43.50 +44:16:09.7 -- not a known variable star
05:37:41.43 +45:58:09.2 -- not a known variable star
05:37:52.51 +43:02:34.8 -- not a known variable star
05:38:24.43 +42:59:47.8 -- not a known variable star
05:38:51.13 +41:49:43.2 -- not a known variable star
05:40:02.66 +50:02:05.9 -- not a known variable star
05:42:07.70 +50:04:31.5 -- not a known variable star
05:43:22.58 +48:15:22.5 -- not a known variable star
05:45:51.93 +50:23:48.2 -- not a known variable star
05:46:26.50 +47:55:01.2 -- not a known variable star
05:46:42.28 +41:24:56.8 -- a known variable star
05:47:45.82 +45:04:51.1 -- not a known variable star
05:48:04.13 +43:19:50.6 -- not a known variable star
05:48:07.96 +49:40:40.2 -- not a known variable star
05:49:29.01 +44:16:19.6 -- not a known variable star
05:53:45.75 +44:06:44.9 -- not a known variable star
05:54:13.34 +47:53:38.5 -- not a known variable star
05:56:58.10 +46:41:29.6 -- not a known variable star
05:57:12.00 +42:33:33.5 -- not a known variable star
06:01:16.82 +47:35:44.4 -- not a known variable star
06:01:30.91 +44:57:14.5 -- not a known variable star
06:01:40.60 +44:57:46.8 -- not a known variable star
06:02:32.13 +48:11:24.3 -- not a known variable star
06:04:15.61 +46:54:36.2 -- not a known variable star
06:07:54.21 +45:58:47.0 -- not a known variable star
06:09:50.60 +49:17:44.2 -- not a known variable star
06:09:51.95 +46:34:27.7 -- a known variable star
06:10:00.20 +45:32:42.1 -- not a known variable star
06:10:45.19 +48:16:56.3 -- not a known variable star
06:12:44.90 +47:30:43.0 -- not a known variable star
06:14:02.99 +50:52:47.6 -- not a known variable star
06:17:09.55 +47:00:39.6 -- not a known variable star
06:17:28.87 +48:00:53.8 -- not a known variable star
06:20:04.37 +46:37:59.6 -- not a known variable star
06:21:48.26 +46:46:31.0 -- not a known variable star
06:23:05.38 +49:11:47.2 -- not a known variable star
06:23:09.77 +49:09:60.0 -- not a known variable star
06:25:49.04 +48:15:43.3 -- not a known variable star
06:26:19.86 +41:59:11.2 -- not a known variable star
06:47:21.13 +48:12:02.0 -- not a known variable star
Found 48 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
52 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 52 (excluding asteroids and hot pixels, 48 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)2461152.65240898 -observatory V36
00:41:36.35 +01:41:08.4 Mercury (-0.2mag)
03:39:04.49 +20:00:39.3 Venus (-3.9mag)
00:35:17.47 +02:46:37.9 Mars (1.2mag)
07:15:37.41 +22:41:11.5 Jupiter (-2.1mag)
00:31:53.59 +01:05:48.0 Saturn (0.9mag)
03:49:01.44 +19:51:42.2 Uranus (5.8mag)
00:11:37.76 -00:10:25.0 Neptune (7.8mag)
20:33:59.18 -22:53:01.2 Pluto (14.5mag)
06:23:54.53 +27:27:05.6 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Apr 21 22:50 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461152.65240898:
07:15:40.82 +22:41:01.7 Io (5.8mag)
07:15:25.66 +22:41:37.6 Europa (5.9mag)
07:15:55.45 +22:40:35.3 Ganymede (5.4mag)
07:15:16.66 +22:41:47.7 Callisto (6.6mag)
07:18:40.32 +22:26:06.7 Himalia (15.4mag)
07:15:37.12 +22:41:09.9 Thebe (16.3mag)
07:18:58.90 +22:56:25.1 Elara (17.3mag)
07:14:55.34 +23:17:58.7 Pasiphae (17.4mag)
07:23:48.45 +22:39:46.2 Carme (18.6mag)
00:31:47.92 +01:05:46.9 Titan (8.8mag)
00:31:59.40 +01:05:49.9 Rhea (10.1mag)
00:31:25.68 +01:04:59.1 Iapetus (11.5mag)
00:31:42.80 +01:06:04.4 Hyperion (14.8mag)
00:33:25.41 +01:13:55.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 21 22:50 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461152.65240898:
16:03:04.59 -20:13:49.6 JWST
17:09:34.86 +43:41:30.7 Chandra
07:58:16.19 -37:43:06.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 21 22:50 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461152.65240898 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:30:08.59 +30:49:45.3 18.0mag P/2009 WX51 (Catalina)
18:54:06.31 -29:09:17.3 13.8mag P/2010 H2 (Vales)
05:11:18.84 -69:22:54.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:52.61 +31:28:54.5 17.3mag C/2017 K2 (PANSTARRS)
17:29:38.11 +11:15:51.9 17.6mag C/2021 G2 (ATLAS)
23:11:43.37 +29:28:59.6 17.1mag C/2022 E2 (ATLAS)
04:36:28.77 +26:12:01.0 16.1mag C/2022 N2 (PANSTARRS)
09:04:59.35 +32:01:52.6 16.3mag C/2022 QE78 (ATLAS)
08:32:12.46 +00:28:37.1 17.4mag C/2022 R6 (PANSTARRS)
18:52:03.37 +19:02:16.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:32.78 -11:25:51.0 17.5mag P/2023 B1 (PANSTARRS)
09:05:05.23 -10:55:31.9 17.7mag C/2023 F3 (ATLAS)
21:59:57.66 +63:16:58.0 17.6mag C/2023 H5 (Lemmon)
19:13:14.92 -03:51:19.7 14.1mag C/2023 R1 (PANSTARRS)
21:12:44.34 +86:46:32.8 17.8mag C/2023 X2 (Lemmon)
06:21:16.19 +63:30:00.0 17.2mag C/2024 A1 (ATLAS)
05:26:02.67 +20:10:28.4 11.4mag C/2024 E1 (Wierzchos)
16:15:07.06 +07:23:25.2 17.3mag C/2024 G6 (ATLAS)
20:22:16.23 +16:58:39.6 14.5mag C/2024 J3 (ATLAS)
03:31:58.75 -21:28:18.1 16.3mag C/2024 T5 (ATLAS)
05:22:03.05 +43:48:39.4 17.7mag C/2025 J1 (Borisov)
13:13:49.73 +48:48:44.4 15.5mag C/2025 L1 (ATLAS)
03:35:17.06 -27:12:32.7 17.9mag C/2025 Q3 (ATLAS)
01:04:18.51 +14:15:53.7 7.8mag C/2025 R3 (PANSTARRS)
12:51:30.15 +03:22:14.4 17.4mag C/2025 Y1 (ATLAS)
04:10:04.07 +02:07:44.5 14.9mag C/2026 A1 (MAPS)
00:16:34.66 +38:16:51.0 14.8mag C/2026 B2 (Sun-Gao)
18:54:52.68 -09:23:01.0 11.5mag 10P/Tempel
14:51:54.83 +02:30:44.9 14.5mag 24P/Schaumasse
11:01:20.40 -01:20:27.4 15.7mag 29P/Schwassmann-Wachmann
10:37:44.78 -03:38:58.2 17.0mag 43P/Wolf-Harrington
01:58:13.42 +18:31:29.6 17.3mag 47P/Ashbrook-Jackson
07:22:23.77 +35:40:07.1 17.0mag 63P/Wild
23:36:46.72 -10:43:36.0 15.7mag 65P/Gunn
04:19:59.89 +23:17:34.0 15.9mag 76P/West-Kohoutek-Ikemura
01:19:16.42 +09:25:32.9 14.3mag 78P/Gehrels
23:21:16.30 -07:34:18.8 14.7mag 88P/Howell
02:28:04.14 +22:14:06.4 15.1mag 93P/Lovas
05:06:41.11 +32:35:39.0 16.1mag 123P/West-Hartley
08:36:03.27 +35:31:47.3 16.2mag 124P/Mrkos
02:42:47.93 +15:02:40.9 16.4mag 128P/Shoemaker-Holt
02:59:39.35 +15:13:11.9 17.5mag 131P/Mueller
01:58:57.51 +15:12:38.7 10.5mag 141P/Machholz
02:06:53.48 +07:09:08.4 10.5mag 141P-A/Machholz
00:49:35.96 +02:54:23.2 12.1mag 141P-D/Machholz
02:37:31.01 +08:53:20.3 17.9mag 141P-I/Machholz
01:19:37.59 +01:34:52.1 15.0mag 162P/SidingSpring
14:40:37.87 +00:29:51.0 17.8mag 210P/Christensen
21:55:55.59 -09:58:55.4 17.8mag 218P/LINEAR
17:17:23.79 -13:10:54.4 16.1mag 235P/LINEAR
05:47:55.55 +35:06:58.0 16.8mag 240P/NEAT
07:41:45.51 -04:31:53.1 17.8mag 242P/Spahr
22:32:18.45 -19:16:46.1 17.7mag 260P/McNaught
02:10:57.55 +21:59:47.7 17.9mag 295P/LINEAR
15:40:01.73 +07:22:22.4 17.5mag 391P/Kowalski
07:36:47.05 +21:22:23.6 17.7mag 450P/LONEOS
05:45:00.08 +44:40:24.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 21 22:50 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
-rw-r--r-- 1 apache apache 5.8K Apr 21 22:50 asassn_transients_list.txt
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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 21 22:50 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:06:16.602 -06:52:59.29 AT 2026jpa 2026-04-13.89 19.276
06:42:32.732 -34:30:04.15 AT 2026joz 2026-04-14.77 18.707
13:06:33.339 -08:24:24.46 AT 2026joy 2026-04-14.02 19.307
21:07:11.613 -12:36:56.09 AT 2026jox 2026-04-14.14 18.849
05:34:42.408 -28:21:31.62 AT 2026jow 2026-04-14.74 18.902
12:30:54.108 -14:11:53.07 AT 2026jov 2026-04-14.03 19.309
05:52:53.155 -34:43:22.49 AT 2026jou 2026-04-14.75 19.398
05:40:18.921 -24:52:33.50 AT 2026jot 2026-04-14.77 18.65
15:53:02.304 +04:30:53.21 AT 2026jos 2026-04-14.09 19.566
11:19:37.053 +36:36:59.54 AT 2026jor 2026-04-11.94 20.14
08:17:15.784 +16:04:01.41 AT 2026joq 2026-04-11.86 19.95
15:52:58.319 -17:01:02.93 AT 2026jop 2026-04-09.53 19.69
09:28:29.338 +17:46:10.46 AT 2026joo 2026-04-11.90 19.1
14:08:31.151 +20:01:29.32 AT 2026jon 2026-04-08.02 19.9
08:15:22.510 -21:29:08.39 AT 2026jom 2026-04-12.37 19.76
12:13:11.990 +05:30:27.70 AT 2026jol 2026-04-08.25 16.6
09:57:55.902 +03:33:01.27 AT 2026jok 2026-03-06.10 21.72
15:47:58.800 -16:07:43.45 AT 2026joj 2026-04-10.44 20.1583
09:57:44.859 +01:08:42.73 AT 2026joi 2026-04-06.02 22.85
14:40:55.647 +05:24:36.73 SN 2026joh 2026-04-14.03 17.708
-rw-r--r-- 1 apache apache 30K Apr 21 22:50 tns_transients_list.txt
