This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM
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 10 12.4946 2461325.9946 9.82 09:13:31.85 -23:23:31.4
251.54118 17.07215 galactic Hya Second-epoch detections are separated by 0.1" and 3.6 pix
The object was found in VSX 0" IQ Hya
Type: M
# Max. Min./Amp. JD0 Period
9.800 V 12.700 V 2452950.00000 385.000000000000 C3,2(Ne)
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 09:13:31.85 -23:23:31.4: 11.22 +/- 0.01 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:13:31.85 -23:23:31.4: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IQ Hya,2461325.9946,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IQ Hya 20261012.4946 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 11.23 09:22:55.39 -30:03:03.9
258.12815 14.15639 galactic Pyx Second-epoch detections are separated by 1.0" and 3.3 pix
The object was found in VSX 1" RV Pyx
Type: M
# Max. Min./Amp. JD0 Period
10.200 V < 14.800 V 2454860.00000 294.500000000000
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 09:22:55.39 -30:03:03.9: 12.94 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:22:55.39 -30:03:03.9: 12.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RV Pyx,2461325.9946,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RV Pyx 20261012.4946 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 11.39 09:25:50.98 -24:00:38.7
253.99900 18.76508 galactic Hya Second-epoch detections are separated by 0.4" and 3.5 pix
The object was found in VSX 3" LP Hya
Type: M
# Max. Min./Amp. JD0 Period
13.000 V < 15.200 V 2452705.00000 465.000000000000 M9
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 09:25:50.98 -24:00:38.7: 13.57 +/- 0.07 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:25:50.98 -24:00:38.7: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LP Hya,2461325.9946,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LP Hya 20261012.4946 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 10.47 09:20:52.78 -27:50:27.0
256.14544 15.34336 galactic Pyx Second-epoch detections are separated by 0.0" and 3.4 pix
The object was found in VSX 1" RS Pyx
Type: M
# Max. Min./Amp. JD0 Period
10.700 V < 15.000 V 2452009.00000 318.000000000000
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 09:20:52.78 -27:50:27.0: 13.94 +/- 0.10 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:20:52.78 -27:50:27.0: 13.89 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RS Pyx,2461325.9946,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RS Pyx 20261012.4946 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 9.24 09:44:58.97 -24:01:16.0
257.25883 21.88719 galactic Hya Second-epoch detections are separated by 0.2" and 3.6 pix
The object was found in VSX 0" RR Hya
Type: M
# Max. Min./Amp. JD0 Period
8.300 V 15.200 V 2454194.00000 343.000000000000 M3.0e-M8e
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 09:44:58.97 -24:01:16.0: 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 09:44:58.97 -24:01:16.0: 12.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 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
RR Hya,2461325.9946,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Hya 20261012.4946 9.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 10.37 09:52:26.73 -23:39:21.3
258.32448 23.32863 galactic Hya Second-epoch detections are separated by 0.5" and 3.5 pix
The object was found in VSX 1" DL Hya
Type: M
# Max. Min./Amp. JD0 Period
12.300 pg < 16.000 pg 2426300.00000 398.000000000000 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 09:52:26.73 -23:39:21.3: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:52:26.73 -23:39:21.3: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DL Hya,2461325.9946,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DL Hya 20261012.4946 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 11.23 09:44:12.80 -30:27:41.2
261.82603 17.09285 galactic Ant Second-epoch detections are separated by 1.2" and 3.1 pix
The object was found in VSX 1" ASAS J094413-3027.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.260 V Y 1.310 V 2452521.40000 487.000000000000
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 09:44:12.80 -30:27:41.2: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:44:12.80 -30:27:41.2: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 10 12.4946* 09 44 12.80 -30 27 41.2 11.2 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 J094413-3027.7,2461325.9946,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J094413-3027.7 20261012.4946 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 12.25 09:52:20.42 -24:50:12.6
259.17740 22.44674 galactic Hya Second-epoch detections are separated by 0.7" and 3.4 pix
The object was found in VSX 2" AH Hya
Type: SR
# Max. Min./Amp. JD0 Period
12.330 V Y 1.250 V 2452146.50000 110.000000000000 :
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 09:52:20.42 -24:50:12.6: 13.59 +/- 0.08 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:52:20.42 -24:50:12.6: 13.79 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AH Hya,2461325.9946,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AH Hya 20261012.4946 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4946 2461325.9946 10.32 09:46:20.07 -29:24:14.9
261.42846 18.18167 galactic Ant Second-epoch detections are separated by 0.2" and 3.4 pix
The object was found in VSX 0" TY Ant
Type: SRB
# Max. Min./Amp. JD0 Period
11.300 V 12.000 V 2452039.20000 103.000000000000
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 09:46:20.07 -29:24:14.9: 11.26 +/- 0.01 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:46:20.07 -29:24:14.9: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.4946* 09 46 20.07 -29 24 14.9 10.3 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
TY Ant,2461325.9946,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TY Ant 20261012.4946 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461325.99488223 12.10.2026 11:52:27.825 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 5 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): 9653
Objects passed selection criteria: 9625
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 6881.75
Average stars matched: 6678.75 (97.0502 %)
Memory usage VmPeak: 235740 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 06:54:35 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 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: 2461325.99488223 12.10.2026 11:52:27.825 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 49
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: 26 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): 69738
Objects passed selection criteria: 69526
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 52177.2
Average stars matched: 50161 (96.1358 %)
Memory usage VmPeak: 289784 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 06:55:41 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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: 2461325.99437645
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits exists and is non-empty
wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits (1st new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Image size: 943.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:00.322 -25:59:43.44 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 09:36:00.322 -25:59:43.44
Angular distance between the image centers 0.0197 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits (2nd new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
Image size: 943.5'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:01.184 -26:00:00.88 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 09:36:01.184 -26:00:00.88
Angular distance between the image centers 0.0143 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 09:36:00.322 -25:59:43.44
Second-epoch second image center 09:36:01.184 -26:00:00.88
Angular distance between the image centers 0.00582 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.wL6czPOseD
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.uQ434ZOY70
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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits &> /tmp/tmp.T24iz6nhcf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits &> /tmp/tmp.e7LvMwKFPm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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 5 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
2.6 pix fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
2.6 pix fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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
13.6 mag. fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
13.5 mag. fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.6 (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.wL6czPOseD (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/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
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.uQ434ZOY70 (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/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
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.T24iz6nhcf (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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_2026-10-12_06-51-44_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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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=331, bad_region=0, passed=3724
Got 3724 stars (including 3391 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat
util/solve_plate_with_UCAC5 got 3724 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.6'
Seting catalog search parameters based on the expected field of view 943.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013106 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010484 (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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 3299 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3283 matched stars entering correct_measured_positions(), 3283 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3283 matched stars entering correct_measured_positions(), 3724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 3299 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3283 matched stars entering correct_measured_positions(), 3724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 3283 matched stars entering correct_measured_positions(), 3724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3283 stars left (next iteration limit 3611)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3283 robust_rms=10.583 arcsec worst_region_rms=21.662 arcsec outer_annulus_rms=21.662 arcsec
SIP_REFIT: SIP order 3 trial: matched=3283 robust_rms=0.735 arcsec worst_region_rms=1.072 arcsec outer_annulus_rms=0.729 arcsec
SIP_REFIT: SIP order 5 trial: matched=3283 robust_rms=0.473 arcsec worst_region_rms=0.570 arcsec outer_annulus_rms=0.491 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3283 robust_rms_before=1.388 arcsec robust_rms_before_corrected=0.390 arcsec robust_rms_after=0.473 arcsec worst_region_rms_before=0.541 worst_region_rms_after=0.570 outer_annulus_rms_before=1.612 outer_annulus_rms_after=0.491
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.541 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits worst_region_rms_kept=0.541 arcsec robust_rms_kept=0.390 arcsec matched=3283
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits N_match=3283 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.401 sigma_q2_arcsec=0.477 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.359 n_q1=1076 n_q2=613 n_q3=906 n_q4=688 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits -region wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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
############ /tmp/tmp.e7LvMwKFPm (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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=330, bad_region=0, passed=3595
Got 3595 stars (including 3261 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat
util/solve_plate_with_UCAC5 got 3595 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.5'
Seting catalog search parameters based on the expected field of view 943.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013104 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010483 (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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 3175 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3161 matched stars entering correct_measured_positions(), 3161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3161 matched stars entering correct_measured_positions(), 3595 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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 3175 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3161 matched stars entering correct_measured_positions(), 3595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 3161 matched stars entering correct_measured_positions(), 3595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 3161 stars left (next iteration limit 3477)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3161 robust_rms=10.853 arcsec worst_region_rms=22.092 arcsec outer_annulus_rms=22.092 arcsec
SIP_REFIT: SIP order 3 trial: matched=3161 robust_rms=0.610 arcsec worst_region_rms=0.864 arcsec outer_annulus_rms=0.736 arcsec
SIP_REFIT: SIP order 5 trial: matched=3161 robust_rms=0.430 arcsec worst_region_rms=0.513 arcsec outer_annulus_rms=0.513 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3161 robust_rms_before=1.337 arcsec robust_rms_before_corrected=0.406 arcsec robust_rms_after=0.430 arcsec worst_region_rms_before=0.545 worst_region_rms_after=0.513 outer_annulus_rms_before=1.539 outer_annulus_rms_after=0.513
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.545 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits worst_region_rms_kept=0.545 arcsec robust_rms_kept=0.406 arcsec matched=3161
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits N_match=3161 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.458 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.379 n_q1=1025 n_q2=601 n_q3=867 n_q4=668 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits -region wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits to local_wcs_cache/
'wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits' -> 'local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits'
Saving the final (post-refit) wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits to local_wcs_cache/
'wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits' -> 'local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits sigma_overall=0.396 worst_q_ratio=1.205
new2=fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits sigma_overall=0.406 worst_q_ratio=1.130
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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554_astrometric_residuals.png (3283 matched stars from wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555_astrometric_residuals.png (3161 matched stars from wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits'
Saving fully-calibrated image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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 09:44:58.97 -24:01:15.9: 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 09:52:26.74 -23:39:21.1: 15.19 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:20:52.78 -27:50:27.1: 13.70 +/- 0.09 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:13:31.85 -23:23:31.4: 11.22 +/- 0.01 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:44:58.97 -24:01:15.9: 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 09:52:26.74 -23:39:21.1: 15.19 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:20:52.78 -27:50:27.1: 13.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Forced photometry filter KEPT candidate at 09:44:58.97 -24:01:15.9: ref_mag=12.32 +/- 0.02 new_mean_mag=9.1069 delta=3.22 (need > 0.90)
Forced photometry filter KEPT candidate at 09:20:52.78 -27:50:27.1: ref_mag=13.66 +/- 0.06 new_mean_mag=10.3337 delta=3.33 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:13:31.85 -23:23:31.4: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Forced photometry filter KEPT candidate at 09:13:31.85 -23:23:31.4: ref_mag=11.23 +/- 0.01 new_mean_mag=9.8204 delta=1.41 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02435.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20680_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 20680_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:44:58.97 -24:01:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.11, MAG_FAINT_SEARCH_LIMIT=10.09)GAIADR2_OUTPUT=# 0.235 5663311273410411520 146.24567516477 -24.02102563228 9.4102 7.6981 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20735_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 20735_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:52:26.74 -23:39:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 0.389 5660766075789768832 148.11152804591 -23.65582527097 9.0371 7.8775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20737_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 20737_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:20:52.78 -27:50:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 0.715 5636775487985674752 140.21969303557 -27.84084329778 10.6846 9.3149 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02435_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 02435_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09221_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 09221_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:51:08.44 -29:53:44.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
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 ####
09:13:31.85 -23:23:31.4
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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits exists and is non-empty
wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits (1st new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Image size: 943.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:00.322 -25:59:43.44 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 09:36:00.322 -25:59:43.44
Angular distance between the image centers 0.0197 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits (2nd new image)
verification OK: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
Image size: 943.5'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:01.184 -26:00:00.88 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 09:36:01.184 -26:00:00.88
Angular distance between the image centers 0.0143 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 09:36:00.322 -25:59:43.44
Second-epoch second image center 09:36:01.184 -26:00:00.88
Angular distance between the image centers 0.00582 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.1pI0HrJEHB
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.ERLQ9HHcdi
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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits &> /tmp/tmp.yXlqclOxc1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits &> /tmp/tmp.JH3xAkakve
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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 47 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
2.5 pix fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
2.5 pix fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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
13.8 mag. fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
13.7 mag. fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
All-image limiting magnitude estimate: 13.7 (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.1pI0HrJEHB (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/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
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.ERLQ9HHcdi (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/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
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.yXlqclOxc1 (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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_2026-10-12_06-51-44_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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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=4, blended=963, bad_region=1, passed=29653
Got 29653 stars (including 28646 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat
util/solve_plate_with_UCAC5 got 29653 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.6'
Seting catalog search parameters based on the expected field of view 943.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013106 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010484 (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 292 to 351 (Dec -31.5 to -20.1)
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: 4840 matched stars entering correct_measured_positions(), 4840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 29653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 292 to 351 (Dec -31.5 to -20.1)
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: 4840 matched stars entering correct_measured_positions(), 29653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 29653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4840 stars left (next iteration limit 5324)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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=4840 robust_rms=10.399 arcsec worst_region_rms=23.286 arcsec outer_annulus_rms=23.286 arcsec
SIP_REFIT: SIP order 3 trial: matched=4840 robust_rms=0.727 arcsec worst_region_rms=1.045 arcsec outer_annulus_rms=0.750 arcsec
SIP_REFIT: SIP order 5 trial: matched=4840 robust_rms=0.481 arcsec worst_region_rms=0.578 arcsec outer_annulus_rms=0.510 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4840 robust_rms_before=1.380 arcsec robust_rms_before_corrected=0.371 arcsec robust_rms_after=0.481 arcsec worst_region_rms_before=0.520 worst_region_rms_after=0.578 outer_annulus_rms_before=1.657 outer_annulus_rms_after=0.510
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.520 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits worst_region_rms_kept=0.520 arcsec robust_rms_kept=0.371 arcsec matched=4840
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits N_match=4840 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.333 sigma_q4_arcsec=0.360 n_q1=1519 n_q2=857 n_q3=1446 n_q4=1018 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits -region wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_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
############ /tmp/tmp.JH3xAkakve (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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
Checking if the catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat corresponding to the image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits
WCS catalog name: wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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=3, blended=836, bad_region=1, passed=28848
Got 28848 stars (including 27967 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat
util/solve_plate_with_UCAC5 got 28848 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.5'
Seting catalog search parameters based on the expected field of view 943.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013104 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010483 (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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4872 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4843 matched stars entering correct_measured_positions(), 28848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4872 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(), 28848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4843 matched stars entering correct_measured_positions(), 28848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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=10.460 arcsec worst_region_rms=23.808 arcsec outer_annulus_rms=23.808 arcsec
SIP_REFIT: SIP order 3 trial: matched=4843 robust_rms=0.618 arcsec worst_region_rms=0.858 arcsec outer_annulus_rms=0.733 arcsec
SIP_REFIT: SIP order 5 trial: matched=4843 robust_rms=0.445 arcsec worst_region_rms=0.520 arcsec outer_annulus_rms=0.520 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4843 robust_rms_before=1.323 arcsec robust_rms_before_corrected=0.378 arcsec robust_rms_after=0.445 arcsec worst_region_rms_before=0.500 worst_region_rms_after=0.520 outer_annulus_rms_before=1.580 outer_annulus_rms_after=0.520
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.500 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits worst_region_rms_kept=0.500 arcsec robust_rms_kept=0.378 arcsec matched=4843
WCS_QUALITY_DIAG: file=fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits N_match=4843 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.448 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.342 n_q1=1519 n_q2=860 n_q3=1441 n_q4=1023 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits -region wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_06-51-44_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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-51-44_20.00sec_-0.00C_LIGHTs_0554.fits
Saving fully-calibrated image wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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_2026-10-12_CI_Ant-01-Q1b1x1_065313_TTUQ1b1x1_2018711_2xWdqjoM/wcs_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555.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 09:03:40.42 -27:55:18.3: 12.17 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:17:02.54 -26:15:15.2: 12.43 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:02:39.82 -26:21:53.2: 13.07 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:02:27.42 -24:56:41.2: 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 09:22:06.43 -29:34:11.8: 15.00 +/- 0.30 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:46:25.82 -25:57:47.8: 11.92 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:06:02.19 -29:15:44.9: 12.01 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:03:40.42 -27:55:18.3: 12.14 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:17:02.54 -26:15:15.2: 12.44 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:02:39.82 -26:21:53.2: 12.95 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:02:27.42 -24:56:41.2: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry filter REJECTED candidate at 09:03:40.42 -27:55:18.3: ref_mag=12.16 +/- 0.02 new_mean_mag=12.2748 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry filter REJECTED candidate at 09:17:02.54 -26:15:15.2: ref_mag=12.43 +/- 0.02 new_mean_mag=12.5705 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:02:39.82 -26:21:53.2: ref_mag=13.00 +/- 0.03 new_mean_mag=13.1212 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:02:27.42 -24:56:41.2: ref_mag=12.66 +/- 0.02 new_mean_mag=12.7498 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 09:46:25.82 -25:57:47.8: 11.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter REJECTED candidate at 09:46:25.82 -25:57:47.8: ref_mag=11.93 +/- 0.01 new_mean_mag=11.6851 delta=0.24 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:22:06.43 -29:34:11.8: 14.65 +/- 0.21 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:09:44.24 -25:49:10.0: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.76 +/- 0.17
Forced photometry filter KEPT candidate at 09:22:06.43 -29:34:11.8: ref_mag=14.76 +/- 0.17 new_mean_mag=11.6496 delta=3.11 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:06:02.19 -29:15:44.9: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Forced photometry filter REJECTED candidate at 09:06:02.19 -29:15:44.9: ref_mag=12.03 +/- 0.01 new_mean_mag=12.0413 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:09:44.24 -25:49:10.0: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry filter REJECTED candidate at 09:09:44.24 -25:49:10.0: ref_mag=12.48 +/- 0.02 new_mean_mag=12.3470 delta=0.14 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:46:20.72 -22:39:56.5: 12.78 +/- 0.04 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:10:51.00 -21:43:35.0: 13.15 +/- 0.05 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:48:36.11 -25:31:39.9: 13.21 +/- 0.06 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:46:20.72 -22:39:56.5: 12.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:22:55.39 -30:03:03.9: 12.94 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 09:46:20.72 -22:39:56.5: ref_mag=12.76 +/- 0.03 new_mean_mag=12.6206 delta=0.14 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:10:51.00 -21:43:35.0: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Forced photometry filter REJECTED candidate at 09:10:51.00 -21:43:35.0: ref_mag=13.06 +/- 0.03 new_mean_mag=13.0858 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:25:50.98 -24:00:38.7: 13.57 +/- 0.07 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:48:36.11 -25:31:39.9: 13.16 +/- 0.06 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:44:58.97 -24:01:16.0: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.04
Forced photometry filter REJECTED candidate at 09:48:36.11 -25:31:39.9: ref_mag=13.19 +/- 0.04 new_mean_mag=13.0057 delta=0.18 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:20:52.78 -27:50:27.0: 13.94 +/- 0.10 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:44:12.80 -30:27:41.2: 12.27 +/- 0.02 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:52:26.73 -23:39:21.3: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:22:55.39 -30:03:03.9: 12.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Forced photometry filter KEPT candidate at 09:22:55.39 -30:03:03.9: ref_mag=12.94 +/- 0.03 new_mean_mag=11.2276 delta=1.72 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:25:50.98 -24:00:38.7: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.05
Forced photometry filter KEPT candidate at 09:25:50.98 -24:00:38.7: ref_mag=13.65 +/- 0.05 new_mean_mag=11.3965 delta=2.25 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:44:58.97 -24:01:16.0: 12.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 09:44:58.97 -24:01:16.0: ref_mag=12.65 +/- 0.02 new_mean_mag=9.2401 delta=3.41 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:20:52.78 -27:50:27.0: 13.89 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.07
Forced photometry filter KEPT candidate at 09:20:52.78 -27:50:27.0: ref_mag=13.91 +/- 0.07 new_mean_mag=10.4743 delta=3.44 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:44:12.80 -30:27:41.2: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Forced photometry filter KEPT candidate at 09:44:12.80 -30:27:41.2: ref_mag=12.26 +/- 0.02 new_mean_mag=11.2320 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:52:26.73 -23:39:21.3: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:52:20.42 -24:50:12.6: 13.59 +/- 0.08 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-28-15_20.00sec_-4.90C_LIGHT_0078.fits at 09:46:20.07 -29:24:14.9: 11.26 +/- 0.01 detection
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:52:20.42 -24:50:12.6: 13.79 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.06
Forced photometry filter KEPT candidate at 09:52:20.42 -24:50:12.6: ref_mag=13.68 +/- 0.06 new_mean_mag=12.2409 delta=1.44 (need > 0.90)
Forced photometry on wcs_Ant-01-Q1b1x1_2026-04-05_22-29-10_20.00sec_-5.00C_LIGHT_0079.fits at 09:46:20.07 -29:24:14.9: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Forced photometry filter KEPT candidate at 09:46:20.07 -29:24:14.9: ref_mag=11.25 +/- 0.01 new_mean_mag=10.3207 delta=0.93 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out92814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out19768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73358.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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: 4s
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Considering the candidate 92462_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92462_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 92467_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92467_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 92468_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92468_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 92471_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92471_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 92472_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92472_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:03:14.07 -26:39:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92474_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92474_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 92475_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92475_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:50:48.70 -26:19:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92568_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92568_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 92602_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92602_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 92768_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92768_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 92780_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92780_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 92814_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92814_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:22:06.43 -29:34:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 2.435 5636279848762936960 140.52606936675 -29.57019506916 12.0887 10.0932 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 92845_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92845_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 92861_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92861_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 92884_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92884_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 92904_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92904_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 92905_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92905_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 92914_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92914_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 92919_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92919_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 92926_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 92926_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:21:32.53 -26:00:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93000_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93000_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 93041_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93041_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:01:47.21 -25:25:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93043_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93043_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 93055_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93055_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:50:51.86 -21:24:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93136_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93136_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 93156_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93156_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 93169_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93169_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:12:25.71 -28:57:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93171_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93171_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 93232_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93232_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 93262_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93262_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 93342_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93342_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 93540_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93540_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
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Considering the candidate 93574_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93574_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 93588_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 93588_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 71275_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 71275_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 59160_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 59160_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 21187_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 21187_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 73358_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 73358_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 21479_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 21479_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 19768_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 19768_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 49664_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 49664_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 28359_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 28359_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 08394_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 08394_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:45:15.17 -22:01:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62827_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
Preparing report for the candidate 62827_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
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Considering the candidate 16851_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 16851_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:13:31.85 -23:23:31.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 29270_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 29270_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
**** FOUND 09:05:04.67 -25:05:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59297_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555
The candidate 59297_fd_Ant-01-Q1b1x1_2026-10-12_06-52-27_20.00sec_0.00C_LIGHTs_0555 did not pass the final checks
