This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL
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 11 03.4799 2461347.9799 11.03 09:22:46.40 -25:55:56.0
254.98514 16.94928 galactic Pyx Second-epoch detections are separated by 0.8" and 17.1 pix
The object was found in VSX 1" RU Pyx
Type: SR
# Max. Min./Amp. JD0 Period
12.530 V Y 1.190 V 2452570.30000 135.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:22:46.40 -25:55:56.0: 12.30 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:22:46.40 -25:55:56.0: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RU Pyx,2461347.9799,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RU Pyx 20261103.4799 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4799 2461347.9799 11.52 09:34:03.73 -27:22:51.2
257.90911 17.76858 galactic Ant Second-epoch detections are separated by 0.8" and 17.1 pix
The object was found in VSX 0" ASAS J093404-2722.9
Type: MISC
# Max. Min./Amp. JD0 Period
12.940 V Y 0.910 V 2452172.40000 136.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:34:03.73 -27:22:51.2: 12.68 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:34:03.73 -27:22:51.2: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 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!
TCP 2026 11 03.4798* 09 34 03.73 -27 22 51.2 11.5 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J093404-2722.9,2461347.9799,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J093404-2722.9 20261103.4799 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4799 2461347.9799 9.22 09:27:24.68 -29:27:17.4
258.38191 15.27182 galactic Pyx Second-epoch detections are separated by 0.4" and 17.3 pix
The object was found in VSX 1" DI Pyx
Type: LB
# Max. Min./Amp. JD0 Period
10.650 V Y 0.760 V 2452530.60000 100.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:27:24.68 -29:27:17.4: 10.34 +/- 0.00 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:27:24.68 -29:27:17.4: 10.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DI Pyx,2461347.9799,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DI Pyx 20261103.4799 9.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4799 2461347.9799 12.85 09:40:04.56 -29:53:57.8
260.74208 16.89102 galactic Ant Second-epoch detections are separated by 1.3" and 17.1 pix
The object was found in VSX 6" SSS_J094005.0-295357
Type: M
# Max. Min./Amp. JD0 Period
9.100 CV 14.200 CV 2454187.00000 450.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:40:04.56 -29:53:57.8: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:40:04.56 -29:53:57.8: 15.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 03.4798* 09 40 04.56 -29 53 57.8 12.8 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SSS_J094005.0-295357,2461347.9799,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J094005.0-295357 20261103.4799 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4799 2461347.9799 11.67 09:16:17.63 -29:36:38.3
256.78698 13.40515 galactic Pyx Second-epoch detections are separated by 0.6" and 17.3 pix
The object was found in VSX 2" X Pyx
Type: M
# Max. Min./Amp. JD0 Period
11.000 V < 14.600 V 2453855.00000 330.000000000000 Me
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:16:17.63 -29:36:38.3: 12.77 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:16:17.63 -29:36:38.3: 12.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 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
X Pyx,2461347.9799,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Pyx 20261103.4799 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4799 2461347.9799 11.70 09:52:09.36 -27:11:11.4
260.84835 20.68376 galactic Ant Second-epoch detections are separated by 1.1" and 16.5 pix
The object was found in VSX 2" ASAS J095209-2711.2
Type: MISC
# Max. Min./Amp. JD0 Period
12.730 V Y 0.970 V 2452149.50000 122.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:52:09.36 -27:11:11.4: 12.63 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:52:09.36 -27:11:11.4: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 03.4798* 09 52 09.36 -27 11 11.4 11.7 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J095209-2711.2,2461347.9799,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J095209-2711.2 20261103.4799 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 11 03.4799 2461347.9799 12.42 09:32:03.31 -28:06:28.5
258.12234 16.94134 galactic Ant Second-epoch detections are separated by 3.2" and 16.7 pix
The object was found in VSX 1" ASASSN-V J093203.32-280627.0
Type: SR
# Max. Min./Amp. JD0 Period
15.300 g Y 0.660 g 2458121.65900 156.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:32:03.31 -28:06:28.5: 13.45 +/- 0.06 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:32:03.31 -28:06:28.5: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 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!
TCP 2026 11 03.4798* 09 32 03.31 -28 06 28.5 12.4 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J093203.32-280627.0,2461347.9799,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J093203.32-280627.0 20261103.4799 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461136.64473718 06.04.2026 03:28:15.292 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
First image: 2461136.64473718 06.04.2026 03:28:15.292 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Last image: 2461347.98013992 03.11.2026 11:31:14.089 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 9987
Objects passed selection criteria: 9980
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 9093
Average stars matched: 8832.5 (97.1352 %)
Memory usage VmPeak: 235760 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 05:36:41 CST 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: 2461136.64473718 06.04.2026 03:28:15.292 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
First image: 2461136.64473718 06.04.2026 03:28:15.292 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Last image: 2461347.98013992 03.11.2026 11:31:14.089 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 46
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 17 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 69710
Objects passed selection criteria: 69513
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 55341.5
Average stars matched: 53109.5 (95.9669 %)
Memory usage VmPeak: 289808 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 05:38:30 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
SExtractor catalog cache: saved Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.cat to cache
SExtractor catalog cache: saved Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.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/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.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: 2461347.97956611
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits exists and is non-empty
wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits exists and is non-empty
wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits exists and is non-empty
wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits (1st reference image)
verification OK: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Image size: 937.5'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:36:04.546 -26:00:25.51 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits (1st new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Image size: 941.3'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: 09:36:01.117 -25:58:36.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:04.546 -26:00:25.51
Second-epoch image center 09:36:01.117 -25:58:36.53
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_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits (2nd new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Image size: 941.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:35:58.787 -25:57:02.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:04.546 -26:00:25.51
Second-epoch image center 09:35:58.787 -25:57:02.30
Angular distance between the image centers 0.0604 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 09:36:01.117 -25:58:36.53
Second-epoch second image center 09:35:58.787 -25:57:02.30
Angular distance between the image centers 0.02759 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/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits &> /tmp/tmp.YC0VIlvkwy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits &> /tmp/tmp.Hg24GczTph
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits &> /tmp/tmp.2jVtbGyUTl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits &> /tmp/tmp.mKvcxBOkGr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Calibrating the magnitude scale
Found non-empty wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.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_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits and wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.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_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits and wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
Found non-empty wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits and wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
The reference image (wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits) and catalog (wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat) found
'wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat' -> 'wcsmag.cat'
Read 10157 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 135.0251 to 153.1714 deg, Dec -31.2864 to -20.4467 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 135.0251 to 153.1714 deg, Dec -31.2864 to -20.4467 deg
Loaded 11311 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): 7501 out of 7795 total matches.
Matched with Tycho-2 7795 out of 10157 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.668500
a=0.000000 b=1.000000 c=22.668500
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.82
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.82
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10157 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 135.0251 to 153.1714 deg, Dec -31.2864 to -20.4467 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 135.0251 to 153.1714 deg, Dec -31.2864 to -20.4467 deg
Loaded 11311 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): 7501 out of 7795 total matches.
Matched with Tycho-2 7795 out of 10157 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Forced-photometry filter: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits -> calib.txt_param_ref_wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits (aperture=6.3)
Read 10198 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 135.0236 to 153.1714 deg, Dec -31.2864 to -20.4478 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 135.0236 to 153.1714 deg, Dec -31.2864 to -20.4478 deg
Loaded 11314 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): 7504 out of 7809 total matches.
Matched with Tycho-2 7809 out of 10198 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Forced-photometry filter: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits -> calib.txt_param_ref_wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
2.3 pix Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
6.6 pix fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
4.2 pix fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Limiting magnitude estimates:
14.8 mag. Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
14.8 mag. Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
14.0 mag. fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
14.3 mag. fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.4 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.YC0VIlvkwy (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/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits' -> 'wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Checking if the catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WCS catalog name: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=750, bad_region=0, passed=10157
Got 10157 stars (including 9401 good ones) from the SExtractor catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
util/solve_plate_with_UCAC5 got 10157 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 10157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 10157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 10157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4849 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits N_match=4849 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.587 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.602 n_q1=1041 n_q2=1237 n_q3=1121 n_q4=1450 worst_quadrant_to_overall_ratio=1.225
WCS_HEADER_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits selection=current_pairs N_selected=4849 N_valid=4849 bias_ra_arcsec=0.002 bias_dec_arcsec=0.004 median_sep_arcsec=0.382 p95_sep_arcsec=2.086 n_q1=1041 n_q2=1237 n_q3=1121 n_q4=1450 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits -region wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Hg24GczTph (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/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits' -> 'wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Checking if the catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WCS catalog name: wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=748, bad_region=1, passed=10198
Got 10198 stars (including 9443 good ones) from the SExtractor catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat
util/solve_plate_with_UCAC5 got 10198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 4856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 10198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 10198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 10198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4855 stars left (next iteration limit 5341)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits N_match=4855 sigma_overall_arcsec=0.506 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.580 sigma_q3_arcsec=0.439 sigma_q4_arcsec=0.612 n_q1=1040 n_q2=1226 n_q3=1120 n_q4=1469 worst_quadrant_to_overall_ratio=1.211
WCS_HEADER_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits selection=current_pairs N_selected=4855 N_valid=4855 bias_ra_arcsec=0.003 bias_dec_arcsec=0.010 median_sep_arcsec=0.394 p95_sep_arcsec=2.037 n_q1=1040 n_q2=1226 n_q3=1120 n_q4=1469 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits -region wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2jVtbGyUTl (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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=231, bad_region=0, passed=7396
Got 7396 stars (including 7164 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat
util/solve_plate_with_UCAC5 got 7396 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 7396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 7396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 7396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 4848 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4848 robust_rms=13.046 arcsec worst_region_rms=27.023 arcsec outer_annulus_rms=27.023 arcsec
SIP_REFIT: SIP order 3 trial: matched=4848 robust_rms=0.704 arcsec worst_region_rms=1.075 arcsec outer_annulus_rms=1.075 arcsec
SIP_REFIT: SIP order 5 trial: matched=4848 robust_rms=0.581 arcsec worst_region_rms=0.794 arcsec outer_annulus_rms=0.794 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4848 robust_rms_before=1.569 arcsec robust_rms_before_corrected=0.612 arcsec robust_rms_after=0.581 arcsec worst_region_rms_before=0.854 worst_region_rms_after=0.794 outer_annulus_rms_before=1.670 outer_annulus_rms_after=0.794
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.854 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits worst_region_rms_kept=0.854 arcsec robust_rms_kept=0.612 arcsec matched=4848
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits N_match=4848 sigma_overall_arcsec=0.605 sigma_q1_arcsec=0.709 sigma_q2_arcsec=0.613 sigma_q3_arcsec=0.624 sigma_q4_arcsec=0.451 n_q1=1434 n_q2=1053 n_q3=1319 n_q4=1042 worst_quadrant_to_overall_ratio=1.171
WCS_HEADER_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits selection=current_pairs N_selected=4848 N_valid=4848 bias_ra_arcsec=0.923 bias_dec_arcsec=0.776 median_sep_arcsec=1.445 p95_sep_arcsec=3.349 n_q1=1434 n_q2=1053 n_q3=1319 n_q4=1042 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits -region wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.mKvcxBOkGr (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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=386, bad_region=0, passed=8831
Got 8831 stars (including 8438 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat
util/solve_plate_with_UCAC5 got 8831 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.2)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 4840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 8831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.2)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 8831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 8831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4841 stars left (next iteration limit 5324)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4841 robust_rms=12.739 arcsec worst_region_rms=26.563 arcsec outer_annulus_rms=26.563 arcsec
SIP_REFIT: SIP order 3 trial: matched=4841 robust_rms=0.514 arcsec worst_region_rms=0.867 arcsec outer_annulus_rms=0.867 arcsec
SIP_REFIT: SIP order 5 trial: matched=4841 robust_rms=0.411 arcsec worst_region_rms=0.681 arcsec outer_annulus_rms=0.681 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4841 robust_rms_before=1.309 arcsec robust_rms_before_corrected=0.410 arcsec robust_rms_after=0.411 arcsec worst_region_rms_before=0.717 worst_region_rms_after=0.681 outer_annulus_rms_before=1.957 outer_annulus_rms_after=0.681
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.717 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits worst_region_rms_kept=0.717 arcsec robust_rms_kept=0.410 arcsec matched=4841
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits N_match=4841 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.507 sigma_q2_arcsec=0.442 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.281 n_q1=1433 n_q2=1039 n_q3=1330 n_q4=1039 worst_quadrant_to_overall_ratio=1.308
WCS_HEADER_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits selection=current_pairs N_selected=4841 N_valid=4841 bias_ra_arcsec=1.025 bias_dec_arcsec=-0.202 median_sep_arcsec=1.174 p95_sep_arcsec=2.976 n_q1=1433 n_q2=1039 n_q3=1330 n_q4=1039 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits -region wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits to local_wcs_cache/
'wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits' -> 'local_wcs_cache/wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits'
Saving the final (post-refit) wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits to local_wcs_cache/
'wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits' -> 'local_wcs_cache/wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits'
Saving the final (post-refit) wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits to local_wcs_cache/
'wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits' -> 'local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits'
Saving the final (post-refit) wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits to local_wcs_cache/
'wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits' -> 'local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits sigma_overall=0.492 worst_q_ratio=1.225
ref2=Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits sigma_overall=0.506 worst_q_ratio=1.211
new1=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits sigma_overall=0.605 worst_q_ratio=1.171
new2=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits sigma_overall=0.388 worst_q_ratio=1.308
reference average sigma_overall=0.499 worst_q_ratio=1.218
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078_astrometric_residuals.png (4849 matched stars from wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079_astrometric_residuals.png (4855 matched stars from wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553_astrometric_residuals.png (4848 matched stars from wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554_astrometric_residuals.png (4841 matched stars from wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits'
Saving fully-calibrated image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits'
Preparing the HTML report for the field Ant-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:39:03.74 -24:52:22.2: 12.16 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:38:12.73 -23:20:23.5: 12.03 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:22:46.40 -25:55:56.0: 12.30 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:32:57.45 -25:41:32.2: 11.63 +/- 0.01 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:34:03.73 -27:22:51.2: 12.68 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:27:24.68 -29:27:17.4: 10.34 +/- 0.00 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:38:12.73 -23:20:23.5: 12.06 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:39:03.74 -24:52:22.2: 12.20 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:22:46.40 -25:55:56.0: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter REJECTED candidate at 09:38:12.73 -23:20:23.5: ref_mag=12.04 +/- 0.01 new_mean_mag=11.4159 delta=0.63 (need > 0.90)
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 09:22:46.40 -25:55:56.0: ref_mag=12.25 +/- 0.02 new_mean_mag=11.0361 delta=1.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:39:03.74 -24:52:22.2: ref_mag=12.18 +/- 0.01 new_mean_mag=11.4587 delta=0.72 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:32:57.45 -25:41:32.2: 11.60 +/- 0.01 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:34:03.73 -27:22:51.2: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter KEPT candidate at 09:34:03.73 -27:22:51.2: ref_mag=12.68 +/- 0.02 new_mean_mag=11.5218 delta=1.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:32:57.45 -25:41:32.2: ref_mag=11.62 +/- 0.01 new_mean_mag=11.5284 delta=0.09 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:27:24.68 -29:27:17.4: 10.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Forced photometry filter KEPT candidate at 09:27:24.68 -29:27:17.4: ref_mag=10.33 +/- 0.00 new_mean_mag=9.2237 delta=1.11 (need > 0.90)
Adding exclusion_list_local.txt__out08066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20854.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 52s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20657_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20657_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:44:58.95 -24:01:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20684_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20684_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:52:26.72 -23:39:21.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20709_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20709_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:22:55.41 -30:03:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20730_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20730_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:25:51.12 -24:00:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20740_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20740_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:20:52.81 -27:50:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20783_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 20783_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20790_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20790_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:45:15.18 -22:01:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20818_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20818_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:22:06.33 -29:34:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20827_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20827_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20836_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20836_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20854_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 20854_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20859_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20859_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20368_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20368_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:44:12.72 -30:27:40.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08066_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 08066_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02435_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 02435_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:13:31.86 -23:23:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09221_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 09221_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:51:08.33 -29:53:43.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 54s
Prepared the HTML report for the field Ant-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:27:24.68 -29:27:17.4
09:22:46.40 -25:55:56.0
09:34:03.73 -27:22:51.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
SExtractor catalog cache: saved Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.cat to cache
SExtractor catalog cache: saved Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Creating symlink local_wcs_cache/wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
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_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits exists and is non-empty
wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits exists and is non-empty
wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits exists and is non-empty
wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits (1st reference image)
verification OK: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Image size: 937.5'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:36:04.546 -26:00:25.51 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits (1st new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Image size: 941.3'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: 09:36:01.117 -25:58:36.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:04.546 -26:00:25.51
Second-epoch image center 09:36:01.117 -25:58:36.53
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_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits (2nd new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Image size: 941.3'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:35:58.787 -25:57:02.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:04.546 -26:00:25.51
Second-epoch image center 09:35:58.787 -25:57:02.30
Angular distance between the image centers 0.0604 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 09:36:01.117 -25:58:36.53
Second-epoch second image center 09:35:58.787 -25:57:02.30
Angular distance between the image centers 0.02759 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/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits &> /tmp/tmp.pAjrJFDDtJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits &> /tmp/tmp.znM7SaSldX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits &> /tmp/tmp.lne74uNTpb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits &> /tmp/tmp.5CTLh4k9rt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Calibrating the magnitude scale
Found non-empty wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.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_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits and wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.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_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits and wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
Found non-empty wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits and wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
The reference image (wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits) and catalog (wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat) found
'wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat' -> 'wcsmag.cat'
Read 75637 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 135.0251 to 153.2145 deg, Dec -31.2936 to -20.4208 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 135.0251 to 153.2145 deg, Dec -31.2936 to -20.4208 deg
Loaded 11361 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): 8443 out of 9507 total matches.
Matched with Tycho-2 9507 out of 75637 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.514700
a=0.000000 b=1.000000 c=22.514700
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 75637 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 135.0251 to 153.2145 deg, Dec -31.2936 to -20.4208 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 135.0251 to 153.2145 deg, Dec -31.2936 to -20.4208 deg
Loaded 11361 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): 8443 out of 9507 total matches.
Matched with Tycho-2 9507 out of 75637 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Forced-photometry filter: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits -> calib.txt_param_ref_wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits (aperture=4.7)
Read 76094 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 135.0236 to 153.2140 deg, Dec -31.3001 to -20.4478 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 135.0236 to 153.2140 deg, Dec -31.3001 to -20.4478 deg
Loaded 11348 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): 8442 out of 9510 total matches.
Matched with Tycho-2 9510 out of 76094 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Forced-photometry filter: calibrated wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits -> calib.txt_param_ref_wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
2.0 pix Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
6.4 pix fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
4.1 pix fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Limiting magnitude estimates:
15.0 mag. Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
15.0 mag. Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
14.0 mag. fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
14.3 mag. fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.0 (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.pAjrJFDDtJ (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/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits' -> 'wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
Checking if the catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits
WCS catalog name: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=33, blended=4401, bad_region=0, passed=75604
Got 75604 stars (including 71115 good ones) from the SExtractor catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat
util/solve_plate_with_UCAC5 got 75604 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 75604 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 75604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 75604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4853 stars left (next iteration limit 5338)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits N_match=4853 sigma_overall_arcsec=0.477 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.570 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.590 n_q1=1034 n_q2=1249 n_q3=1119 n_q4=1451 worst_quadrant_to_overall_ratio=1.237
WCS_HEADER_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits selection=current_pairs N_selected=4853 N_valid=4853 bias_ra_arcsec=-0.018 bias_dec_arcsec=-0.001 median_sep_arcsec=0.377 p95_sep_arcsec=1.977 n_q1=1034 n_q2=1249 n_q3=1119 n_q4=1451 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits -region wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.znM7SaSldX (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/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits' -> 'wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
Checking if the catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat corresponding to the image wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits
WCS catalog name: wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=37, blended=4411, bad_region=3, passed=76057
Got 76057 stars (including 71551 good ones) from the SExtractor catalog wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat
util/solve_plate_with_UCAC5 got 76057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 4861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 76057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 76057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 76057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4861 stars left (next iteration limit 5347)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits N_match=4861 sigma_overall_arcsec=0.494 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.565 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.595 n_q1=1027 n_q2=1260 n_q3=1116 n_q4=1458 worst_quadrant_to_overall_ratio=1.205
WCS_HEADER_DIAG: file=Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits selection=current_pairs N_selected=4861 N_valid=4861 bias_ra_arcsec=-0.023 bias_dec_arcsec=0.005 median_sep_arcsec=0.391 p95_sep_arcsec=1.907 n_q1=1027 n_q2=1260 n_q3=1116 n_q4=1458 occupied_cells_4x4=16/16
The image catalog is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits -region wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lne74uNTpb (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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=36, blended=2872, bad_region=31, passed=30068
Got 30068 stars (including 27159 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat
util/solve_plate_with_UCAC5 got 30068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4843 matched stars entering correct_measured_positions(), 4843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4843 matched stars entering correct_measured_positions(), 30068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4843 matched stars entering correct_measured_positions(), 30068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4843 matched stars entering correct_measured_positions(), 30068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 4843 stars left (next iteration limit 5327)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4843 robust_rms=13.070 arcsec worst_region_rms=26.916 arcsec outer_annulus_rms=26.916 arcsec
SIP_REFIT: SIP order 3 trial: matched=4843 robust_rms=0.696 arcsec worst_region_rms=1.057 arcsec outer_annulus_rms=1.057 arcsec
SIP_REFIT: SIP order 5 trial: matched=4843 robust_rms=0.573 arcsec worst_region_rms=0.782 arcsec outer_annulus_rms=0.782 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4843 robust_rms_before=1.558 arcsec robust_rms_before_corrected=0.599 arcsec robust_rms_after=0.573 arcsec worst_region_rms_before=0.834 worst_region_rms_after=0.782 outer_annulus_rms_before=1.660 outer_annulus_rms_after=0.782
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.834 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits worst_region_rms_kept=0.834 arcsec robust_rms_kept=0.599 arcsec matched=4843
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits N_match=4843 sigma_overall_arcsec=0.606 sigma_q1_arcsec=0.719 sigma_q2_arcsec=0.588 sigma_q3_arcsec=0.607 sigma_q4_arcsec=0.466 n_q1=1428 n_q2=1060 n_q3=1298 n_q4=1057 worst_quadrant_to_overall_ratio=1.188
WCS_HEADER_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits selection=current_pairs N_selected=4843 N_valid=4843 bias_ra_arcsec=0.917 bias_dec_arcsec=0.770 median_sep_arcsec=1.441 p95_sep_arcsec=3.292 n_q1=1428 n_q2=1060 n_q3=1298 n_q4=1057 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits -region wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.5CTLh4k9rt (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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=2284, bad_region=35, passed=41442
Got 41442 stars (including 39098 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat
util/solve_plate_with_UCAC5 got 41442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.2)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 4846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 41442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.2)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 41442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 41442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4847 stars left (next iteration limit 5330)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4847 robust_rms=12.776 arcsec worst_region_rms=26.756 arcsec outer_annulus_rms=26.756 arcsec
SIP_REFIT: SIP order 3 trial: matched=4847 robust_rms=0.515 arcsec worst_region_rms=0.855 arcsec outer_annulus_rms=0.855 arcsec
SIP_REFIT: SIP order 5 trial: matched=4847 robust_rms=0.412 arcsec worst_region_rms=0.654 arcsec outer_annulus_rms=0.654 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4847 robust_rms_before=1.308 arcsec robust_rms_before_corrected=0.398 arcsec robust_rms_after=0.412 arcsec worst_region_rms_before=0.679 worst_region_rms_after=0.654 outer_annulus_rms_before=1.932 outer_annulus_rms_after=0.654
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.679 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits worst_region_rms_kept=0.679 arcsec robust_rms_kept=0.398 arcsec matched=4847
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits N_match=4847 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.323 sigma_q4_arcsec=0.294 n_q1=1383 n_q2=1028 n_q3=1352 n_q4=1084 worst_quadrant_to_overall_ratio=1.258
WCS_HEADER_DIAG: file=fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits selection=current_pairs N_selected=4847 N_valid=4847 bias_ra_arcsec=1.022 bias_dec_arcsec=-0.213 median_sep_arcsec=1.172 p95_sep_arcsec=2.910 n_q1=1383 n_q2=1028 n_q3=1352 n_q4=1084 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits -region wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-30-24_20.00sec_-0.00C_LIGHTs_0553.fits
Saving fully-calibrated image wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.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_2026-11-03_CI_Ant-01-Q1b1x1_053201_TTUQ1b1x1_1482851_wLBYJ1YL/wcs_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554.fits
Preparing the HTML report for the field Ant-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:11:03.29 -27:29:17.5: 13.01 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:40:32.28 -24:29:34.8: 13.67 +/- 0.07 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:18:10.73 -21:41:38.3: 13.29 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 10:06:19.80 -21:12:02.4: 13.25 +/- 0.07 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:30:41.97 -29:06:50.7: 13.03 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:24:51.75 -28:06:17.5: 12.76 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:30:44.56 -26:23:28.3: 13.04 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:48:38.63 -26:22:01.1: 13.42 +/- 0.07 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:42:08.72 -27:13:33.1: 13.21 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:27:45.12 -23:24:07.1: 13.45 +/- 0.06 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:30:44.56 -26:23:28.3: 13.08 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:48:38.63 -26:22:01.1: 13.39 +/- 0.06 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:18:10.73 -21:41:38.3: 13.25 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:30:41.97 -29:06:50.7: 12.95 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:11:03.29 -27:29:17.5: 13.01 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 10:06:19.80 -21:12:02.4: 13.22 +/- 0.07 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:42:08.72 -27:13:33.1: 13.21 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:24:51.75 -28:06:17.5: 12.65 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:40:32.28 -24:29:34.8: 13.58 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Forced photometry reference-image weighted average: 13.23 +/- 0.05
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Forced photometry filter REJECTED candidate at 09:30:44.56 -26:23:28.3: ref_mag=13.06 +/- 0.03 new_mean_mag=13.0220 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter REJECTED candidate at 09:18:10.73 -21:41:38.3: ref_mag=13.27 +/- 0.04 new_mean_mag=13.1530 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:06:19.80 -21:12:02.4: ref_mag=13.23 +/- 0.05 new_mean_mag=13.2113 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Forced photometry filter REJECTED candidate at 09:30:41.97 -29:06:50.7: ref_mag=12.99 +/- 0.03 new_mean_mag=12.9056 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.21 +/- 0.04
Forced photometry filter REJECTED candidate at 09:48:38.63 -26:22:01.1: ref_mag=13.40 +/- 0.05 new_mean_mag=13.4106 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:11:03.29 -27:29:17.5: ref_mag=13.01 +/- 0.03 new_mean_mag=12.9713 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:24:51.75 -28:06:17.5: ref_mag=12.70 +/- 0.02 new_mean_mag=12.8600 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:40:32.28 -24:29:34.8: ref_mag=13.62 +/- 0.05 new_mean_mag=13.2547 delta=0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:42:08.72 -27:13:33.1: ref_mag=13.21 +/- 0.04 new_mean_mag=13.0525 delta=0.16 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:27:45.12 -23:24:07.1: 13.58 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter REJECTED candidate at 09:27:45.12 -23:24:07.1: ref_mag=13.51 +/- 0.04 new_mean_mag=13.2437 delta=0.27 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:58:15.30 -30:58:34.4: 12.54 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:20:49.84 -23:48:42.0: 12.86 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:19:56.53 -30:01:25.1: 12.36 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:02:04.53 -27:36:14.9: 13.05 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:28:28.40 -21:49:28.8: 12.90 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:17:16.14 -28:51:48.2: 12.35 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:14:01.60 -25:05:06.3: 12.66 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:29:21.84 -21:18:01.3: 13.19 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:38:35.30 -20:59:10.4: 13.22 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:06:04.65 -28:37:19.1: 12.65 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:29:21.84 -21:18:01.3: 13.12 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:38:35.30 -20:59:10.4: 13.16 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:17:16.14 -28:51:48.2: 12.31 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:20:49.84 -23:48:42.0: 12.87 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:28:28.40 -21:49:28.8: 12.84 +/- 0.03 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:14:01.60 -25:05:06.3: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:19:56.53 -30:01:25.1: 12.40 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 09:29:21.84 -21:18:01.3: ref_mag=13.15 +/- 0.03 new_mean_mag=12.8323 delta=0.32 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:58:15.30 -30:58:34.4: 12.62 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:02:04.53 -27:36:14.9: 13.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter REJECTED candidate at 09:38:35.30 -20:59:10.4: ref_mag=13.18 +/- 0.03 new_mean_mag=12.9019 delta=0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter REJECTED candidate at 09:17:16.14 -28:51:48.2: ref_mag=12.33 +/- 0.02 new_mean_mag=12.3702 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:20:49.84 -23:48:42.0: ref_mag=12.86 +/- 0.02 new_mean_mag=12.7927 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Forced photometry filter REJECTED candidate at 09:28:28.40 -21:49:28.8: ref_mag=12.87 +/- 0.02 new_mean_mag=12.9092 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:14:01.60 -25:05:06.3: ref_mag=12.68 +/- 0.02 new_mean_mag=12.7116 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.57 +/- 0.03
Forced photometry filter REJECTED candidate at 09:19:56.53 -30:01:25.1: ref_mag=12.38 +/- 0.02 new_mean_mag=12.3549 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Forced photometry filter REJECTED candidate at 09:58:15.30 -30:58:34.4: ref_mag=12.57 +/- 0.03 new_mean_mag=12.5201 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:02:04.53 -27:36:14.9: ref_mag=13.05 +/- 0.04 new_mean_mag=12.7581 delta=0.29 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:06:04.65 -28:37:19.1: 12.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.03
Forced photometry filter REJECTED candidate at 09:06:04.65 -28:37:19.1: ref_mag=12.65 +/- 0.03 new_mean_mag=12.3529 delta=0.30 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:21:37.82 -30:11:00.5: 12.21 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:59:14.43 -26:11:10.6: 12.97 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:40:04.56 -29:53:57.8: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:16:17.63 -29:36:38.3: 12.77 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:59:14.43 -26:11:10.6: 12.92 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:52:09.36 -27:11:11.4: 12.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.04
Forced photometry filter REJECTED candidate at 09:59:14.43 -26:11:10.6: ref_mag=12.94 +/- 0.04 new_mean_mag=12.6480 delta=0.29 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:21:37.82 -30:11:00.5: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry filter REJECTED candidate at 09:21:37.82 -30:11:00.5: ref_mag=12.18 +/- 0.02 new_mean_mag=12.0818 delta=0.10 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:40:04.56 -29:53:57.8: 15.26 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:16:17.63 -29:36:38.3: 12.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
Forced photometry filter KEPT candidate at 09:16:17.63 -29:36:38.3: ref_mag=12.82 +/- 0.03 new_mean_mag=11.6721 delta=1.15 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:52:09.36 -27:11:11.4: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter KEPT candidate at 09:52:09.36 -27:11:11.4: ref_mag=12.63 +/- 0.02 new_mean_mag=11.6986 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:32:03.31 -28:06:28.5: 13.45 +/- 0.06 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:32:03.31 -28:06:28.5: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 09:32:03.31 -28:06:28.5: ref_mag=13.47 +/- 0.04 new_mean_mag=12.4261 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out54685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71754.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 92478_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92478_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92484_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92484_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92501_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92501_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92525_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92525_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:09:02.87 -22:18:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92528_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92528_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92530_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92530_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92537_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92537_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92538_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92538_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92552_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92552_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92562_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92562_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92571_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92571_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92594_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92594_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92598_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92598_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92603_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92603_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92613_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92613_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92633_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92633_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92657_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92657_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92666_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92666_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92676_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92676_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92690_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92690_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92700_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92700_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92710_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92710_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 92713_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92713_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:04:16.38 -30:32:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92893_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 92893_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:22:06.38 -29:34:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93286_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 93286_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
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Considering the candidate 59160_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 59160_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:22:55.40 -30:03:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59990_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 59990_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
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Considering the candidate 54330_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 54330_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:34:03.73 -27:22:50.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 21187_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 21187_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:25:51.13 -24:00:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73358_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 73358_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:20:52.81 -27:50:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61963_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 61963_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
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Considering the candidate 21479_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 21479_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:44:58.95 -24:01:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54685_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 54685_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
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Considering the candidate 19768_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 19768_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:52:26.71 -23:39:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35305_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 35305_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:22:46.41 -25:55:56.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 49664_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 49664_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:44:12.71 -30:27:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28359_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 28359_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:52:20.42 -24:50:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06421_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 06421_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:34:47.43 -21:52:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71754_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
Preparing report for the candidate 71754_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
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Considering the candidate 08394_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 08394_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:45:15.14 -22:01:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16851_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 16851_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:13:31.86 -23:23:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20058_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 20058_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:03:53.52 -23:49:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63138_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 63138_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
**** FOUND 09:27:24.69 -29:27:17.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59297_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554
The candidate 59297_fd_Ant-01-Q1b1x1_2026-11-03_05-31-14_20.00sec_-0.00C_LIGHTs_0554 did not pass the final checks
