This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN
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 07 12.4263 2461233.9263 12.29 05:45:01.71 +38:39:40.3
171.61787 4.95037 galactic Aur Second-epoch detections are separated by 1.8" and 5.6 pix
The object was found in VSX 2" V0735 Aur
Type: LB
# Max. Min./Amp. JD0 Period
11.350 R1 11.600 R1
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:01.71 +38:39:40.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:01.71 +38:39:40.3: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0735 Aur,2461233.9263,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0735 Aur 20260712.4263 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.15 05:41:01.08 +34:37:15.1
174.64711 2.15188 galactic Aur Second-epoch detections are separated by 2.6" and 5.8 pix
The object was found in VSX 1" V0341 Aur
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 14.000 V 350.000000000000 : C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:41:01.08 +34:37:15.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:41:01.08 +34:37:15.1: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 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
V0341 Aur,2461233.9263,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0341 Aur 20260712.4263 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.54 05:20:44.92 +38:10:49.3
169.43229 0.69883 galactic Aur Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in VSX 1" V0487 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.000 pg 14.100 pg 8.779630000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:44.92 +38:10:49.3: 13.88 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:44.92 +38:10:49.3: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0487 Aur,2461233.9263,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0487 Aur 20260712.4263 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.60 05:38:03.74 +34:25:03.4
174.49553 1.52817 galactic Aur Second-epoch detections are separated by 5.3" and 5.4 pix
The object was found in VSX 2" NSVS 6981396
Type: SR
# Max. Min./Amp. JD0 Period
15.361 g Y 0.605 g 2458592.76150 92.345619800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:38:03.74 +34:25:03.4: 14.07 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:38:03.74 +34:25:03.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 6981396,2461233.9263,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6981396 20260712.4263 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.72 05:25:29.61 +35:35:43.7
172.10065 0.01942 galactic Aur Second-epoch detections are separated by 3.5" and 5.6 pix
The object was found in VSX 1" ASASSN-V J052529.57+353544.7
Type: L
# Max. Min./Amp. JD0 Period
14.120 V 14.960 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:29.61 +35:35:43.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:29.61 +35:35:43.7: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052529.57+353544.7,2461233.9263,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052529.57+353544.7 20260712.4263 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 07 12.4263 2461233.9263 11.74 05:41:19.64 +41:19:09.7
168.96676 5.72542 galactic Aur Second-epoch detections are separated by 0.4" and 5.3 pix
The object was found in VSX 4" V0368 Aur
Type: SR
# Max. Min./Amp. JD0 Period
13.700 pg 14.500 pg
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:41:19.64 +41:19:09.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:41:19.64 +41:19:09.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0368 Aur,2461233.9263,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0368 Aur 20260712.4263 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.52 05:37:14.62 +39:16:26.5
170.29772 3.98448 galactic Aur Second-epoch detections are separated by 1.1" and 5.4 pix
The object was found in VSX 6" ZTF J053714.82+391632.4
Type: SR
# Max. Min./Amp. JD0 Period
12.356 r Y 0.671 r 2458430.07640 172.528106800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:14.62 +39:16:26.5: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:14.62 +39:16:26.5: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053714.82+391632.4,2461233.9263,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J053714.82+391632.4 20260712.4263 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.28 05:47:58.73 +41:17:44.5
169.63354 6.78443 galactic Aur Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX 2" ASASSN-V J054758.83+411746.1
Type: L
# Max. Min./Amp. JD0 Period
13.420 V 14.060 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:58.73 +41:17:44.5: 13.40 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:58.73 +41:17:44.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054758.83+411746.1,2461233.9263,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J054758.83+411746.1 20260712.4263 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.00 04:59:47.82 +35:03:05.0
169.45840 -4.54038 galactic Aur Second-epoch detections are separated by 1.5" and 5.3 pix
The object was found in VSX 7" V0472 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.800 pg 14.100 pg 199.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:59:47.82 +35:03:05.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:59:47.82 +35:03:05.0: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.05 +/- 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
V0472 Aur,2461233.9263,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0472 Aur 20260712.4263 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.04 05:09:44.61 +40:44:23.4
166.11472 0.46371 galactic Aur Second-epoch detections are separated by 2.0" and 5.2 pix
The object was found in VSX 1" V0478 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
12.200 pg 13.500 pg 50.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:09:44.61 +40:44:23.4: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:09:44.61 +40:44:23.4: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0478 Aur,2461233.9263,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0478 Aur 20260712.4263 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 12.4263 2461233.9263 12.57 05:26:53.92 +35:34:48.6
172.27305 0.24773 galactic Aur Second-epoch detections are separated by 1.9" and 5.1 pix
The object was found in VSX 1" ASASSN-V J052653.96+353448.1
Type: SR
# Max. Min./Amp. JD0 Period
13.850 V 14.680 V 2458363.21340 348.303522200000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:26:53.92 +35:34:48.6: 13.96 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:26:53.92 +35:34:48.6: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052653.96+353448.1,2461233.9263,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052653.96+353448.1 20260712.4263 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461233.92651523 12.07.2026 10:14:00.916 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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): 16798
Objects passed selection criteria: 16700
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 13457.8
Average stars matched: 11823.8 (87.8583 %)
Memory usage VmPeak: 129488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jul 11 21:08:03 CDT 2026
VaST build number 1.0rc89-146-gb95cfcf3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 12 07:16:24 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: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461233.92651523 12.07.2026 10:14:00.916 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 149
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 50 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): 131559
Objects passed selection criteria: 131228
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 111140
Average stars matched: 95934 (86.3182 %)
Memory usage VmPeak: 1981604 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Jul 11 21:08:03 CDT 2026
VaST build number 1.0rc89-146-gb95cfcf3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 12 07:20:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461233.92604031
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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits'
wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.024 +37:59:58.79 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Image size: 942.7'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:27:25.133 +37:58:49.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:25.133 +37:58:49.18
Angular distance between the image centers 0.0329 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Image size: 942.6'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:27:26.483 +37:59:16.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:26.483 +37:59:16.92
Angular distance between the image centers 0.0332 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:25.133 +37:58:49.18
Second-epoch second image center 05:27:26.483 +37:59:16.92
Angular distance between the image centers 0.00889 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.FmeYpwvPxC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.EgwUtSXXyb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits &> /tmp/tmp.ED2wQyv1dj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits &> /tmp/tmp.g45cZv3VVA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8766 to 92.1250 deg, Dec +31.9889 to +43.3926 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 70.8766 to 92.1250 deg, Dec 31.9889 to 43.3926 deg
Loaded 16031 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): 11098 out of 12445 total matches.
Matched with Tycho-2 12445 out of 27843 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.926900
a=0.000000 b=1.000000 c=22.926900
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8766 to 92.1250 deg, Dec +31.9889 to +43.3926 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 70.8766 to 92.1250 deg, Dec 31.9889 to 43.3926 deg
Loaded 16031 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): 11098 out of 12445 total matches.
Matched with Tycho-2 12445 out of 27843 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.2)
Read 27116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3508 to 92.6935 deg, Dec +32.1410 to +43.3194 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 71.3508 to 92.6935 deg, Dec 32.1410 to 43.3194 deg
Loaded 16021 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): 10961 out of 12446 total matches.
Matched with Tycho-2 12446 out of 27116 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.3 pix fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
2.2 pix fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
2.2 pix wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
15.2 mag. Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.2 mag. Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.3 mag. fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
13.4 mag. fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.7 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FmeYpwvPxC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2982, bad_region=5998, passed=27843
Got 27843 stars (including 19362 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 27843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 22185 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 22185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 22185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=949 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.529 sigma_q2_arcsec=0.378 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.332 n_q1=219 n_q2=218 n_q3=308 n_q4=204 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EgwUtSXXyb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3147, bad_region=5347, passed=27116
Got 27116 stars (including 19176 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 27116 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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21725 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21725 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21725 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=944 sigma_overall_arcsec=0.557 sigma_q1_arcsec=0.642 sigma_q2_arcsec=0.513 sigma_q3_arcsec=0.463 sigma_q4_arcsec=0.583 n_q1=267 n_q2=215 n_q3=286 n_q4=176 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ED2wQyv1dj (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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=362, bad_region=697, passed=6007
Got 6007 stars (including 4985 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat
util/solve_plate_with_UCAC5 got 6007 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 5287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 5287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 5287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits N_match=941 sigma_overall_arcsec=0.748 sigma_q1_arcsec=0.725 sigma_q2_arcsec=0.759 sigma_q3_arcsec=0.774 sigma_q4_arcsec=0.737 n_q1=249 n_q2=129 n_q3=393 n_q4=170 worst_quadrant_to_overall_ratio=1.035
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits -region wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.g45cZv3VVA (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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=351, bad_region=704, passed=5895
Got 5895 stars (including 4876 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 5895 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 5174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 5171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 5171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits N_match=942 sigma_overall_arcsec=0.720 sigma_q1_arcsec=0.728 sigma_q2_arcsec=0.746 sigma_q3_arcsec=0.738 sigma_q4_arcsec=0.719 n_q1=249 n_q2=133 n_q3=388 n_q4=172 worst_quadrant_to_overall_ratio=1.036
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits -region wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits sigma_overall=0.441 worst_q_ratio=1.201
ref2=Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits sigma_overall=0.557 worst_q_ratio=1.152
new1=fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits sigma_overall=0.748 worst_q_ratio=1.035
new2=fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits sigma_overall=0.720 worst_q_ratio=1.036
reference average sigma_overall=0.499 worst_q_ratio=1.1765
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049_astrometric_residuals.png (949 matched stars from wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054_astrometric_residuals.png (944 matched stars from wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454_astrometric_residuals.png (941 matched stars from wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455_astrometric_residuals.png (942 matched stars from wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits'
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36474_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 36474_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:26:54.58 +36:54:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36483_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 36483_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:07:57.12 +37:48:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14476_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 14476_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:41:55.70 +38:55:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06908_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 06908_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:19.06 +35:15:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14902_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 14902_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:49:09.97 +39:10:49.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-03-Q2b1x1 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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking 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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.024 +37:59:58.79 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Image size: 942.7'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:27:25.133 +37:58:49.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:25.133 +37:58:49.18
Angular distance between the image centers 0.0329 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Image size: 942.6'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:27:26.483 +37:59:16.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:26.483 +37:59:16.92
Angular distance between the image centers 0.0332 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:25.133 +37:58:49.18
Second-epoch second image center 05:27:26.483 +37:59:16.92
Angular distance between the image centers 0.00889 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.L9AxypucQM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.qWR1cXVIQz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits &> /tmp/tmp.tygdADKQfm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits &> /tmp/tmp.t9a8IdXaER
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8154 to 92.1472 deg, Dec +31.9889 to +43.3931 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 70.8154 to 92.1472 deg, Dec 31.9889 to 43.3931 deg
Loaded 16059 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): 8333 out of 12787 total matches.
Matched with Tycho-2 12787 out of 202315 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774400
a=0.000000 b=1.000000 c=22.774400
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8154 to 92.1472 deg, Dec +31.9889 to +43.3931 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 70.8154 to 92.1472 deg, Dec 31.9889 to 43.3931 deg
Loaded 16059 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): 8333 out of 12787 total matches.
Matched with Tycho-2 12787 out of 202315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=4.6)
Read 212259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3349 to 92.7190 deg, Dec +32.1410 to +43.3202 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 71.3349 to 92.7190 deg, Dec 32.1410 to 43.3202 deg
Loaded 16044 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): 8107 out of 12844 total matches.
Matched with Tycho-2 12844 out of 212259 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 114 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.2 pix fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
2.1 pix fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
2.1 pix wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.5 mag. Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.7 mag. fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
13.7 mag. fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.L9AxypucQM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=30655, bad_region=36141, passed=202270
Got 202270 stars (including 139401 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 202270 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 167780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 167781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 167784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=944 sigma_overall_arcsec=0.447 sigma_q1_arcsec=0.492 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.386 n_q1=219 n_q2=214 n_q3=315 n_q4=196 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qWR1cXVIQz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=32150, bad_region=35314, passed=212204
Got 212204 stars (including 148997 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 212204 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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 177772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 177771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 177772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=941 sigma_overall_arcsec=0.567 sigma_q1_arcsec=0.653 sigma_q2_arcsec=0.514 sigma_q3_arcsec=0.460 sigma_q4_arcsec=0.624 n_q1=285 n_q2=195 n_q3=303 n_q4=158 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tygdADKQfm (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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3437, bad_region=4718, passed=56188
Got 56188 stars (including 48259 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat
util/solve_plate_with_UCAC5 got 56188 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 51366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 51366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 51367 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits N_match=940 sigma_overall_arcsec=0.756 sigma_q1_arcsec=0.752 sigma_q2_arcsec=0.817 sigma_q3_arcsec=0.765 sigma_q4_arcsec=0.732 n_q1=259 n_q2=124 n_q3=386 n_q4=171 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits -region wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.t9a8IdXaER (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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3051, bad_region=4812, passed=57427
Got 57427 stars (including 49725 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 57427 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 52453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 52451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 52451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits N_match=941 sigma_overall_arcsec=0.752 sigma_q1_arcsec=0.738 sigma_q2_arcsec=0.835 sigma_q3_arcsec=0.788 sigma_q4_arcsec=0.671 n_q1=260 n_q2=123 n_q3=383 n_q4=175 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits -region wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-13-19_20.00sec_5.00C_LIGHT_0454.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.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_2026-07-12_CI_Aur-03-Q2b1x1_062338_TTUQ2b1x1_3209190_5AUTxYcN/wcs_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455.fits
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:56.67 +37:28:25.1: 13.02 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:18.57 +37:01:20.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:19.58 +39:11:49.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:28:21.83 +34:45:57.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:29.31 +39:42:20.3: 12.42 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:02:50.19 +33:29:06.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:56.67 +37:28:25.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter REJECTED candidate at 05:20:56.67 +37:28:25.1: ref_mag=13.08 +/- 0.02 new_mean_mag=13.1437 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:19.58 +39:11:49.3: 12.94 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:18.57 +37:01:20.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter REJECTED candidate at 05:18:19.58 +39:11:49.3: ref_mag=12.94 +/- 0.01 new_mean_mag=13.0753 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter REJECTED candidate at 05:27:18.57 +37:01:20.8: ref_mag=12.90 +/- 0.01 new_mean_mag=12.8972 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:57:16.65 +40:54:42.6: 13.02 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:02:50.19 +33:29:06.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:28:21.83 +34:45:57.2: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 05:02:50.19 +33:29:06.2: ref_mag=12.82 +/- 0.02 new_mean_mag=12.8739 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter REJECTED candidate at 05:28:21.83 +34:45:57.2: ref_mag=12.80 +/- 0.02 new_mean_mag=12.9716 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:16.79 +38:10:48.2: 12.27 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:40.10 +36:16:44.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:29.31 +39:42:20.3: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 05:45:29.31 +39:42:20.3: ref_mag=12.45 +/- 0.01 new_mean_mag=12.5809 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:57:16.65 +40:54:42.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:16.79 +38:10:48.2: 12.32 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 04:57:16.65 +40:54:42.6: ref_mag=13.02 +/- 0.03 new_mean_mag=13.1530 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter REJECTED candidate at 05:47:16.79 +38:10:48.2: ref_mag=12.30 +/- 0.01 new_mean_mag=12.3372 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:40.10 +36:16:44.9: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:52.17 +42:14:45.1: 12.48 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 05:32:40.10 +36:16:44.9: ref_mag=13.16 +/- 0.02 new_mean_mag=12.7180 delta=0.44 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:55:00.27 +40:31:46.5: 13.35 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:36.54 +37:35:32.8: 13.20 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:34:08.47 +39:56:56.4: 12.43 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:52.17 +42:14:45.1: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter REJECTED candidate at 05:37:52.17 +42:14:45.1: ref_mag=12.53 +/- 0.01 new_mean_mag=12.4796 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:02:12.60 +38:50:06.3: 12.71 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:55:00.27 +40:31:46.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.35 +/- 0.04
Forced photometry filter REJECTED candidate at 04:55:00.27 +40:31:46.5: ref_mag=13.35 +/- 0.04 new_mean_mag=13.2289 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:36.54 +37:35:32.8: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter REJECTED candidate at 05:01:36.54 +37:35:32.8: ref_mag=13.20 +/- 0.03 new_mean_mag=12.9618 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:34:08.47 +39:56:56.4: 12.48 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:02:51.23 +40:20:52.6: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 05:34:08.47 +39:56:56.4: ref_mag=12.45 +/- 0.01 new_mean_mag=12.4579 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:03:18.24 +39:12:38.8: 12.82 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:58:31.36 +40:46:22.2: 9.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:02:12.60 +38:50:06.3: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 05:02:12.60 +38:50:06.3: ref_mag=12.71 +/- 0.02 new_mean_mag=12.7840 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:03:18.24 +39:12:38.8: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 05:03:18.24 +39:12:38.8: ref_mag=12.82 +/- 0.02 new_mean_mag=12.7862 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:02:51.23 +40:20:52.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:58:31.36 +40:46:22.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 9.76 +/- 0.00
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter REJECTED candidate at 05:02:51.23 +40:20:52.6: ref_mag=12.14 +/- 0.01 new_mean_mag=12.3048 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:58:31.36 +40:46:22.2: ref_mag=9.76 +/- 0.00 new_mean_mag=10.0922 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:54:15.87 +41:08:27.4: 12.31 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:28.90 +40:30:32.3: 12.66 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:10.62 +41:14:48.4: 12.79 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:54:15.87 +41:08:27.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 04:54:15.87 +41:08:27.4: ref_mag=12.31 +/- 0.01 new_mean_mag=12.4417 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:28.90 +40:30:32.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:58:54.55 +41:03:06.2: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Forced photometry filter REJECTED candidate at 05:01:28.90 +40:30:32.3: ref_mag=12.66 +/- 0.03 new_mean_mag=12.4748 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:35:58.11 +41:01:34.0: 12.25 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:10.62 +41:14:48.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.79 +/- 0.03
Forced photometry filter REJECTED candidate at 05:01:10.62 +41:14:48.4: ref_mag=12.79 +/- 0.03 new_mean_mag=12.6532 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:58:54.55 +41:03:06.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Forced photometry filter REJECTED candidate at 04:58:54.55 +41:03:06.2: ref_mag=12.99 +/- 0.03 new_mean_mag=12.8886 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:35:58.11 +41:01:34.0: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 05:35:58.11 +41:01:34.0: ref_mag=12.19 +/- 0.01 new_mean_mag=12.5113 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:02:02.04 +41:20:03.5: 13.18 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:41.63 +41:49:33.9: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:00:37.47 +40:15:22.5: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:02:02.04 +41:20:03.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry filter REJECTED candidate at 05:02:02.04 +41:20:03.5: ref_mag=13.18 +/- 0.03 new_mean_mag=13.0476 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:41.63 +41:49:33.9: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 05:17:41.63 +41:49:33.9: ref_mag=12.82 +/- 0.02 new_mean_mag=12.8347 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:00:37.47 +40:15:22.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter REJECTED candidate at 05:00:37.47 +40:15:22.5: ref_mag=13.09 +/- 0.03 new_mean_mag=13.1798 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:39.76 +38:45:56.8: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:39.76 +38:45:56.8: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Forced photometry filter REJECTED candidate at 05:01:39.76 +38:45:56.8: ref_mag=13.27 +/- 0.04 new_mean_mag=13.2177 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:03:20.38 +36:34:49.9: 14.10 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:03:36.23 +40:29:40.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:01.71 +38:39:40.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:03:20.38 +36:34:49.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:03:36.23 +40:29:40.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Forced photometry filter KEPT candidate at 05:03:20.38 +36:34:49.9: ref_mag=14.10 +/- 0.06 new_mean_mag=12.8578 delta=1.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:44.92 +38:10:49.3: 13.88 +/- 0.05 detection
Forced photometry filter KEPT candidate at 05:03:36.23 +40:29:40.5: ref_mag=13.31 +/- 0.03 new_mean_mag=12.0999 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:41:01.08 +34:37:15.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:38:03.74 +34:25:03.4: 14.07 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:01.71 +38:39:40.3: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 05:45:01.71 +38:39:40.3: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2858 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:44.92 +38:10:49.3: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry filter KEPT candidate at 05:20:44.92 +38:10:49.3: ref_mag=13.96 +/- 0.04 new_mean_mag=12.5411 delta=1.41 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:41:01.08 +34:37:15.1: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 05:41:01.08 +34:37:15.1: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1526 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:29.61 +35:35:43.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:38:03.74 +34:25:03.4: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry filter KEPT candidate at 05:38:03.74 +34:25:03.4: ref_mag=13.96 +/- 0.04 new_mean_mag=12.5952 delta=1.36 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:29.61 +35:35:43.7: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 05:25:29.61 +35:35:43.7: ref_mag=13.77 +/- 0.03 new_mean_mag=12.7079 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:41:19.64 +41:19:09.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:14.62 +39:16:26.5: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:14.62 +39:16:26.5: 13.68 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:41:19.64 +41:19:09.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 05:41:19.64 +41:19:09.7: ref_mag=12.85 +/- 0.02 new_mean_mag=11.7418 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 05:37:14.62 +39:16:26.5: ref_mag=13.71 +/- 0.03 new_mean_mag=12.5158 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:58.73 +41:17:44.5: 13.40 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:58.73 +41:17:44.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 05:47:58.73 +41:17:44.5: ref_mag=13.36 +/- 0.02 new_mean_mag=12.2633 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:59:47.82 +35:03:05.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:59:47.82 +35:03:05.0: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 04:59:47.82 +35:03:05.0: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0008 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:09:44.61 +40:44:23.4: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:09:44.61 +40:44:23.4: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 05:09:44.61 +40:44:23.4: ref_mag=13.08 +/- 0.02 new_mean_mag=12.0365 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:26:53.92 +35:34:48.6: 13.96 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:26:53.92 +35:34:48.6: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 05:26:53.92 +35:34:48.6: ref_mag=13.66 +/- 0.03 new_mean_mag=12.5504 delta=1.11 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out150761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96748.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 7s
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Considering the candidate 272017_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272017_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272026_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272026_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272029_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272029_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:04:20.19 +39:36:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272034_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272034_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272038_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272038_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 272040_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272040_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272041_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272041_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:11:21.89 +40:34:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272045_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272045_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272046_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272046_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:20:27.18 +35:39:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272047_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272047_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272048_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272048_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:21:21.07 +35:28:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272049_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272049_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272056_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272056_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272057_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272057_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272062_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272062_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272064_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272064_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272068_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272068_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272070_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272070_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:36:28.25 +34:07:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272073_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272073_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:21:21.12 +38:51:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272075_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272075_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272080_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272080_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272081_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272081_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272088_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272088_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272091_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272091_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:04:36.86 +39:49:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272095_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272095_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272127_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272127_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:19:15.70 +40:07:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272169_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272169_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:13:19.93 +38:30:50.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272176_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272176_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:24:42.97 +37:25:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272206_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272206_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:10:27.41 +37:19:04.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272222_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272222_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:19:49.19 +40:57:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272231_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272231_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:17.98 +33:47:34.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272242_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272242_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:24:47.25 +37:21:51.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272269_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272269_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272272_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272272_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:19:01.53 +41:06:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272274_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272274_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:26:50.86 +38:58:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272280_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272280_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:27:41.44 +34:26:43.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272284_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272284_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272290_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272290_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:17:19.65 +39:28:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272301_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272301_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:14:49.46 +39:31:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272320_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272320_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:49:06.56 +39:13:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272330_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272330_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272343_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272343_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:30:54.22 +39:49:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272347_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272347_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:24:49.89 +37:22:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272375_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272375_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272388_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272388_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
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Considering the candidate 272435_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272435_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:13:46.37 +41:12:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272436_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272436_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:02:43.72 +41:05:36.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 272453_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272453_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:32.00 +40:27:41.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272455_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272455_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:00:09.26 +39:38:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272456_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272456_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:00:11.06 +39:24:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272466_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272466_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:20:45.73 +38:30:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272467_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272467_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:06:24.79 +41:11:56.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 272485_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272485_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:09:36.41 +38:39:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272491_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272491_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:06:33.85 +35:29:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272497_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272497_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272517_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272517_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:13:15.99 +40:10:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272568_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272568_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272572_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272572_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:45:47.13 +40:29:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272586_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272586_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:32:38.88 +39:32:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272587_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272587_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:26:40.54 +34:23:17.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 272606_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272606_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:28.27 +37:36:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272615_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272615_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272617_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272617_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:14:44.97 +39:31:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272632_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272632_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:17:58.00 +35:10:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272637_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272637_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:07:48.50 +39:51:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272660_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272660_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:15:04.63 +35:21:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272695_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272695_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:14:43.72 +41:23:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272702_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272702_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:10:18.47 +40:22:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272729_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272729_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:06:28.79 +35:34:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272732_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272732_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272737_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272737_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:10:58.17 +39:16:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272742_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272742_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:06:42.37 +39:53:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272745_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272745_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:39:56.44 +37:58:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272748_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272748_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:09:34.68 +34:52:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272758_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272758_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:20:49.21 +37:27:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272761_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272761_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:30:14.57 +40:29:51.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272778_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272778_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:39.91 +39:21:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272779_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272779_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:06:20.13 +41:15:42.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272788_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272788_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:46.69 +40:24:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272791_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272791_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:08:09.70 +36:07:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272802_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272802_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:28:10.87 +39:10:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272806_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272806_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:44:55.80 +38:31:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272809_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272809_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:35:43.55 +38:03:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272821_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272821_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:30:42.95 +39:52:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272824_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272824_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:08:39.88 +37:35:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272827_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272827_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:29:49.55 +35:22:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272831_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 272831_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:22:17.02 +37:03:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32333_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 32333_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 04:59:52.84 +33:59:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73667_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 73667_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:03:20.38 +36:34:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.879 186446866782255232 075.83444515566 +36.58088704708 11.5019 9.9973 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102240_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 102240_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150761_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 150761_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:03:36.23 +40:29:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.106 200840126828455808 075.90019251121 +40.49452718966 12.1056 11.0739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32190_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 32190_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96748_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 96748_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111430_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 111430_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:41:55.61 +38:55:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29050_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 29050_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102689_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 102689_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:32:02.24 +38:38:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114669_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 114669_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:20:15.03 +39:06:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50292_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 50292_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
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Considering the candidate 194777_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 194777_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
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Considering the candidate 46899_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 46899_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:18:19.04 +35:15:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114580_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 114580_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95220_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 95220_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:07:57.12 +37:48:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72927_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 72927_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:26:54.58 +36:54:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195170_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 195170_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
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Considering the candidate 86440_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 86440_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:30:32.85 +37:44:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49989_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 49989_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
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Considering the candidate 198845_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 198845_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
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Considering the candidate 49874_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
Preparing report for the candidate 49874_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
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Considering the candidate 84748_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 84748_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:24:39.31 +37:23:06.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 138800_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 138800_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:19:09.94 +40:05:35.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 133126_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 133126_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:24:55.81 +40:04:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35080_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 35080_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:27:38.96 +34:28:34.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 26464_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 26464_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
**** FOUND 05:20:00.98 +33:57:30.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116001_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455
The candidate 116001_fd_Aur-03-Q2b1x1_2026-07-12_05-14-00_20.00sec_5.00C_LIGHT_0455 did not pass the final checks
