This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph
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 09 18.2396 2461301.7396 11.33 22:15:18.50 -13:18:37.8
45.78116 -51.05435 galactic Aqr Second-epoch detections are separated by 0.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5 Astraea -0 -0 0 11.5 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:15:18.50 -13:18:37.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:15:18.50 -13:18:37.8: 15.70 +/- 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
VARIABLE_NAME,2461301.7396,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 12.27 22:31:05.22 -12:17:20.0
50.25114 -53.96117 galactic Aqr Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.117 Lomia -0 -0 0 12.5 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:05.22 -12:17:20.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:05.22 -12:17:20.0: 15.76 +/- 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
VARIABLE_NAME,2461301.7396,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 12.97 22:05:02.74 -10:44:50.7
47.46181 -47.63852 galactic Aqr Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.78 Diana 0 -0 0 13.0 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:05:02.74 -10:44:50.7: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:05:02.74 -10:44:50.7: 15.89 +/- 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
VARIABLE_NAME,2461301.7396,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 13.45 22:35:14.23 -09:55:36.0
54.56393 -53.60676 galactic Aqr Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.208 Lacrimosa -0 0 0 13.5 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:35:14.23 -09:55:36.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:35:14.23 -09:55:36.0: 15.75 +/- 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
VARIABLE_NAME,2461301.7396,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 13.48 22:18:47.43 -11:14:10.3
49.32044 -50.82378 galactic Aqr Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.303 Josephina 0 -0 0 13.7 -0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:18:47.43 -11:14:10.3: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:18:47.43 -11:14:10.3: 15.86 +/- 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
VARIABLE_NAME,2461301.7396,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 14.11 22:27:33.41 -09:13:19.5
53.85285 -51.63322 galactic Aqr Second-epoch detections are separated by 1.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.846 Lipperta -0 -0 0 14.3 0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:27:33.41 -09:13:19.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:27:33.41 -09:13:19.5: 15.88 +/- 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
VARIABLE_NAME,2461301.7396,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 14.20 22:13:33.79 -14:14:11.2
44.16135 -51.08544 galactic Aqr Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1331 Solvejg 1 0 1 14.4 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:13:33.79 -14:14:11.2: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:13:33.79 -14:14:11.2: 15.78 +/- 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
VARIABLE_NAME,2461301.7396,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 14.54 22:42:59.82 -11:21:05.5
54.26170 -55.98054 galactic Aqr Second-epoch detections are separated by 1.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1386 Storeria -1 -0 1 14.8 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:59.82 -11:21:05.5: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:59.82 -11:21:05.5: 15.56 +/- 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
VARIABLE_NAME,2461301.7396,14.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 14.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 18.2396 2461301.7396 14.59 22:40:37.57 -11:05:17.2
54.10643 -55.34831 galactic Aqr Second-epoch detections are separated by 1.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2271 Kiso -0 -0 0 14.7 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:40:37.57 -11:05:17.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:40:37.57 -11:05:17.2: 15.64 +/- 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
VARIABLE_NAME,2461301.7396,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260918.2396 14.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
First image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461301.73990863 18.09.2026 05:45:18.106 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 7 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): 5536
Objects passed selection criteria: 5531
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 5246.75
Average stars matched: 5032.5 (95.9165 %)
Memory usage VmPeak: 232720 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Sep 18 01:41:46 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: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
First image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461301.73990863 18.09.2026 05:45:18.106 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 82
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 52 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): 34248
Objects passed selection criteria: 34154
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 32628
Average stars matched: 31341 (96.0555 %)
Memory usage VmPeak: 257976 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Sep 18 01:43:53 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461301.73933021
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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.412 -09:59:39.54 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.522 -09:59:47.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:08.522 -09:59:47.86
Angular distance between the image centers 0.0375 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Image size: 936.9'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:05.633 -09:59:21.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:05.633 -09:59:21.89
Angular distance between the image centers 0.0260 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 22:17:08.522 -09:59:47.86
Second-epoch second image center 22:17:05.633 -09:59:21.89
Angular distance between the image centers 0.01388 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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.dsowHy5UP8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.SCpVdzizkB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits &> /tmp/tmp.5jYFiQttvo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits &> /tmp/tmp.NIG1bWebV9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat' -> 'wcsmag.cat'
Read 6925 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 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 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Loaded 5569 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): 4112 out of 4275 total matches.
Matched with Tycho-2 4275 out of 6925 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.666700
a=0.000000 b=1.000000 c=22.666700
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.18
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6925 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 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 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Loaded 5569 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): 4112 out of 4275 total matches.
Matched with Tycho-2 4275 out of 6925 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=5.7)
Read 6918 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8535 to 342.3813 deg, Dec -15.6029 to -4.2885 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 325.8535 to 342.3813 deg, Dec -15.6029 to -4.2885 deg
Loaded 5525 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): 4139 out of 4302 total matches.
Matched with Tycho-2 4302 out of 6918 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=5.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.1 pix Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Limiting magnitude estimates:
15.2 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.2 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.1 mag. fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
15.1 mag. fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.dsowHy5UP8 (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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=496, bad_region=1750, passed=6925
Got 6925 stars (including 4788 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 6925 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4148 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 4126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 5503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4148 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 5503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 5503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4126 stars left (next iteration limit 4538)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4126 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.337 n_q1=1267 n_q2=739 n_q3=1220 n_q4=900 worst_quadrant_to_overall_ratio=1.321
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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.SCpVdzizkB (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/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=479, bad_region=1750, passed=6918
Got 6918 stars (including 4798 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 6918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4150 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4130 matched stars entering correct_measured_positions(), 4130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4129 matched stars entering correct_measured_positions(), 5496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4149 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4129 matched stars entering correct_measured_positions(), 5496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4129 matched stars entering correct_measured_positions(), 5496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4129 stars left (next iteration limit 4541)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4129 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.317 n_q1=1265 n_q2=760 n_q3=1216 n_q4=888 worst_quadrant_to_overall_ratio=1.291
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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.5jYFiQttvo (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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=498, bad_region=1873, passed=7275
Got 7275 stars (including 4988 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat
util/solve_plate_with_UCAC5 got 7275 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4343 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4319 matched stars entering correct_measured_positions(), 4319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4319 matched stars entering correct_measured_positions(), 5779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4345 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4320 matched stars entering correct_measured_positions(), 5779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4320 matched stars entering correct_measured_positions(), 5779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4320 stars left (next iteration limit 4750)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4320 robust_rms=7.461 arcsec worst_quadrant_rms=8.533 arcsec
SIP_REFIT: SIP order 3 trial: matched=4320 robust_rms=0.375 arcsec worst_quadrant_rms=0.426 arcsec
SIP_REFIT: SIP order 5 trial: matched=4320 robust_rms=0.317 arcsec worst_quadrant_rms=0.329 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4320 robust_rms_before=0.852 arcsec robust_rms_before_corrected=0.323 arcsec robust_rms_after=0.317 arcsec worst_quadrant_rms_before=0.338 worst_quadrant_rms_after=0.329
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.338 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits N_match=4320 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.344 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.357 n_q1=1317 n_q2=892 n_q3=1192 n_q4=919 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.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.NIG1bWebV9 (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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=483, bad_region=1864, passed=7298
Got 7298 stars (including 5032 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat
util/solve_plate_with_UCAC5 got 7298 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4340 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 4318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 5813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4342 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4319 matched stars entering correct_measured_positions(), 5813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4319 matched stars entering correct_measured_positions(), 5813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4319 stars left (next iteration limit 4749)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4319 robust_rms=7.461 arcsec worst_quadrant_rms=8.205 arcsec
SIP_REFIT: SIP order 3 trial: matched=4319 robust_rms=0.362 arcsec worst_quadrant_rms=0.415 arcsec
SIP_REFIT: SIP order 5 trial: matched=4319 robust_rms=0.302 arcsec worst_quadrant_rms=0.323 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4319 robust_rms_before=0.848 arcsec robust_rms_before_corrected=0.323 arcsec robust_rms_after=0.302 arcsec worst_quadrant_rms_before=0.346 worst_quadrant_rms_after=0.323
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.346 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits N_match=4319 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.338 n_q1=1306 n_q2=882 n_q3=1201 n_q4=930 worst_quadrant_to_overall_ratio=1.044
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
Saving the final (post-refit) wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits sigma_overall=0.361 worst_q_ratio=1.321
ref2=Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits sigma_overall=0.341 worst_q_ratio=1.291
new1=fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits sigma_overall=0.348 worst_q_ratio=1.048
new2=fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits sigma_overall=0.346 worst_q_ratio=1.044
reference average sigma_overall=0.351 worst_q_ratio=1.306
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859_astrometric_residuals.png (4126 matched stars from wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860_astrometric_residuals.png (4129 matched stars from wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260_astrometric_residuals.png (4320 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261_astrometric_residuals.png (4319 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:46.98 -08:09:26.9: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:17:21.96 -09:35:11.4: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:22:11.87 -09:21:06.2: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:44.67 -08:12:17.0: 12.09 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:15:18.50 -13:18:37.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:17:21.96 -09:35:11.4: 12.04 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:15:18.50 -13:18:37.8: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:46.98 -08:09:26.9: 12.02 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 22:17:21.96 -09:35:11.4: ref_mag=12.04 +/- 0.01 new_mean_mag=12.0245 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:44.67 -08:12:17.0: 12.09 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:22:11.87 -09:21:06.2: 12.00 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 22:23:46.98 -08:09:26.9: ref_mag=12.04 +/- 0.01 new_mean_mag=12.0279 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 22:22:11.87 -09:21:06.2: ref_mag=12.00 +/- 0.01 new_mean_mag=11.9686 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:16:44.67 -08:12:17.0: ref_mag=12.09 +/- 0.01 new_mean_mag=12.0515 delta=0.04 (need > 0.90)
Adding exclusion_list_local.txt__out20364.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20364_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 20364_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20384_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 20384_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
**** FOUND 22:04:39.86 -07:11:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20401_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 20401_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20408_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 20408_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20409_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 20409_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20412_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 20412_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:15:18.50 -13:18:37.8
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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.412 -09:59:39.54 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.522 -09:59:47.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:08.522 -09:59:47.86
Angular distance between the image centers 0.0375 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Image size: 936.9'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:05.633 -09:59:21.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:16:59.412 -09:59:39.54
Second-epoch image center 22:17:05.633 -09:59:21.89
Angular distance between the image centers 0.0260 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 22:17:08.522 -09:59:47.86
Second-epoch second image center 22:17:05.633 -09:59:21.89
Angular distance between the image centers 0.01388 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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.BC8yzriiBG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.j9ihq6cd9U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits &> /tmp/tmp.YmKlRLsETv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits &> /tmp/tmp.v3hzlZicTr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat' -> 'wcsmag.cat'
Read 44007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 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 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Loaded 5591 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): 4073 out of 4476 total matches.
Matched with Tycho-2 4476 out of 44007 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.559400
a=0.000000 b=1.000000 c=22.559400
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 44007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 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 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Loaded 5591 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): 4073 out of 4476 total matches.
Matched with Tycho-2 4476 out of 44007 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=4.5)
Read 43933 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8257 to 342.4191 deg, Dec -15.6029 to -4.2242 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 325.8257 to 342.4191 deg, Dec -15.6029 to -4.2242 deg
Loaded 5583 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): 4085 out of 4489 total matches.
Matched with Tycho-2 4489 out of 43933 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=4.5)
____ 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 Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.0 pix Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.1 pix fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
2.1 pix fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Limiting magnitude estimates:
15.4 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.3 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.3 mag. fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
15.3 mag. fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.5 (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.BC8yzriiBG (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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1813, bad_region=10057, passed=43988
Got 43988 stars (including 32499 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 43988 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 4297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 36021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 36021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 36021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4297 stars left (next iteration limit 4726)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4297 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.438 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.314 n_q1=1364 n_q2=840 n_q3=1218 n_q4=875 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.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.j9ihq6cd9U (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/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1714, bad_region=10072, passed=43917
Got 43917 stars (including 32478 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 43917 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 4295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 35918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4315 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 35918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 35918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4295 stars left (next iteration limit 4724)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4295 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.284 sigma_q4_arcsec=0.303 n_q1=1376 n_q2=836 n_q3=1205 n_q4=878 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.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.YmKlRLsETv (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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1836, bad_region=7667, passed=39615
Got 39615 stars (including 30641 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat
util/solve_plate_with_UCAC5 got 39615 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4321 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4300 matched stars entering correct_measured_positions(), 4300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4300 matched stars entering correct_measured_positions(), 33812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4322 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4300 matched stars entering correct_measured_positions(), 33812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4300 matched stars entering correct_measured_positions(), 33811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4300 stars left (next iteration limit 4730)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.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=4300 robust_rms=7.240 arcsec worst_quadrant_rms=8.733 arcsec
SIP_REFIT: SIP order 3 trial: matched=4300 robust_rms=0.370 arcsec worst_quadrant_rms=0.414 arcsec
SIP_REFIT: SIP order 5 trial: matched=4300 robust_rms=0.312 arcsec worst_quadrant_rms=0.322 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4300 robust_rms_before=0.843 arcsec robust_rms_before_corrected=0.319 arcsec robust_rms_after=0.312 arcsec worst_quadrant_rms_before=0.328 worst_quadrant_rms_after=0.322
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.328 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits N_match=4300 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.347 n_q1=1347 n_q2=860 n_q3=1211 n_q4=882 worst_quadrant_to_overall_ratio=1.041
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.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.v3hzlZicTr (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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1847, bad_region=7655, passed=39359
Got 39359 stars (including 30377 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat
util/solve_plate_with_UCAC5 got 39359 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4311 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 4293 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 33613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4312 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 33613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 33613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4293 stars left (next iteration limit 4722)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.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=4293 robust_rms=7.245 arcsec worst_quadrant_rms=8.786 arcsec
SIP_REFIT: SIP order 3 trial: matched=4293 robust_rms=0.354 arcsec worst_quadrant_rms=0.399 arcsec
SIP_REFIT: SIP order 5 trial: matched=4293 robust_rms=0.296 arcsec worst_quadrant_rms=0.313 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4293 robust_rms_before=0.832 arcsec robust_rms_before_corrected=0.311 arcsec robust_rms_after=0.296 arcsec worst_quadrant_rms_before=0.330 worst_quadrant_rms_after=0.313
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.330 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits N_match=4293 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.289 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.317 n_q1=1338 n_q2=867 n_q3=1219 n_q4=869 worst_quadrant_to_overall_ratio=1.043
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.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_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-44-28_20.00sec_-0.00C_LIGHT_0260.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.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_2026-09-18_CI_Aqr-04-Q2b1x1_005416_TTUQ2b1x1_4104435_aa2fSYph/wcs_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261.fits
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:05.22 -12:17:20.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:00:32.41 -10:14:15.9: 14.22 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:11:04.72 -08:09:05.5: 13.85 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:48.34 -09:41:01.0: 14.73 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:28:49.11 -13:16:15.2: 14.54 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:40:35.35 -13:16:22.0: 14.85 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:07:21.15 -09:35:52.9: 14.73 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:05:02.74 -10:44:50.7: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:35:14.23 -09:55:36.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:18:47.43 -11:14:10.3: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:07:21.15 -09:35:52.9: 14.78 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.09
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:48.34 -09:41:01.0: 14.57 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 22:07:21.15 -09:35:52.9: ref_mag=14.75 +/- 0.09 new_mean_mag=14.8680 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:05.22 -12:17:20.0: 15.76 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.64 +/- 0.10
Forced photometry filter REJECTED candidate at 22:41:48.34 -09:41:01.0: ref_mag=14.64 +/- 0.10 new_mean_mag=14.4955 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:00:32.41 -10:14:15.9: 14.17 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:05:02.74 -10:44:50.7: 15.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Forced photometry filter REJECTED candidate at 22:00:32.41 -10:14:15.9: ref_mag=14.19 +/- 0.06 new_mean_mag=14.3242 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:35:14.23 -09:55:36.0: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:40:35.35 -13:16:22.0: 15.04 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:28:49.11 -13:16:15.2: 14.72 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.15
Forced photometry reference-image weighted average: 14.62 +/- 0.09
Forced photometry filter REJECTED candidate at 22:28:49.11 -13:16:15.2: ref_mag=14.62 +/- 0.09 new_mean_mag=14.6750 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:40:35.35 -13:16:22.0: ref_mag=14.93 +/- 0.15 new_mean_mag=14.8166 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:11:04.72 -08:09:05.5: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Forced photometry filter REJECTED candidate at 22:11:04.72 -08:09:05.5: ref_mag=13.82 +/- 0.04 new_mean_mag=14.0006 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:18:47.43 -11:14:10.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:37:59.64 -12:52:30.1: 14.65 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:13:33.79 -14:14:11.2: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:34:47.11 -11:22:27.7: 14.43 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:27:33.41 -09:13:19.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:25.58 -11:55:11.1: 14.63 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:37:59.64 -12:52:30.1: 14.87 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:13:33.79 -14:14:11.2: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.74 +/- 0.12
Forced photometry filter REJECTED candidate at 22:37:59.64 -12:52:30.1: ref_mag=14.74 +/- 0.12 new_mean_mag=14.4856 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:34:47.11 -11:22:27.7: 14.36 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.08
Forced photometry filter REJECTED candidate at 22:34:47.11 -11:22:27.7: ref_mag=14.39 +/- 0.08 new_mean_mag=14.3972 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:27:33.41 -09:13:19.5: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:25.58 -11:55:11.1: 14.68 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:36.04 -13:42:43.6: 14.84 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.11
Forced photometry filter REJECTED candidate at 22:41:25.58 -11:55:11.1: ref_mag=14.66 +/- 0.11 new_mean_mag=14.5069 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:36.04 -13:42:43.6: 14.87 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.13
Forced photometry filter REJECTED candidate at 22:36:36.04 -13:42:43.6: ref_mag=14.85 +/- 0.13 new_mean_mag=14.5039 delta=0.35 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:59.82 -11:21:05.5: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:24.88 -14:04:25.3: 15.02 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:40:37.57 -11:05:17.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:59.82 -11:21:05.5: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:24.88 -14:04:25.3: 14.68 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:43:45.53 -11:30:22.8: 14.47 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.14
Forced photometry filter REJECTED candidate at 22:42:24.88 -14:04:25.3: ref_mag=14.80 +/- 0.14 new_mean_mag=14.5249 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:40:37.57 -11:05:17.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:43:45.53 -11:30:22.8: 14.72 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.11
Forced photometry filter REJECTED candidate at 22:43:45.53 -11:30:22.8: ref_mag=14.57 +/- 0.11 new_mean_mag=14.5668 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:42.53 -12:31:04.3: 15.02 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:53.42 -12:39:25.2: 15.18 +/- 0.28 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:42.53 -12:31:04.3: 14.85 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.14
Forced photometry filter REJECTED candidate at 22:39:42.53 -12:31:04.3: ref_mag=14.93 +/- 0.14 new_mean_mag=14.7119 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:53.42 -12:39:25.2: 14.78 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.15
Forced photometry filter REJECTED candidate at 22:44:53.42 -12:39:25.2: ref_mag=14.91 +/- 0.15 new_mean_mag=14.6795 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:21:11.59 -13:32:12.9: 15.23 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:01.64 -09:51:04.7: 15.15 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:21:11.59 -13:32:12.9: 15.06 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.14
Forced photometry filter REJECTED candidate at 22:21:11.59 -13:32:12.9: ref_mag=15.13 +/- 0.14 new_mean_mag=14.7995 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:01.64 -09:51:04.7: 15.06 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.15
Forced photometry filter REJECTED candidate at 22:39:01.64 -09:51:04.7: ref_mag=15.10 +/- 0.15 new_mean_mag=14.7978 delta=0.30 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:36.95 -12:05:37.3: 14.92 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:36.95 -12:05:37.3: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.13
Forced photometry filter REJECTED candidate at 22:44:36.95 -12:05:37.3: ref_mag=14.75 +/- 0.13 new_mean_mag=14.7011 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:30:51.71 -12:16:17.3: 15.27 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:30:51.71 -12:16:17.3: 15.54 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.18
Forced photometry filter REJECTED candidate at 22:30:51.71 -12:16:17.3: ref_mag=15.37 +/- 0.18 new_mean_mag=14.8128 delta=0.56 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:00:08.22 -13:02:52.3: 15.03 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:00:08.22 -13:02:52.3: 15.17 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.14
Forced photometry filter REJECTED candidate at 22:00:08.22 -13:02:52.3: ref_mag=15.09 +/- 0.14 new_mean_mag=14.7531 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:02:12.23 -13:02:39.1: 15.26 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:02:12.23 -13:02:39.1: 14.80 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.13
Forced photometry filter REJECTED candidate at 22:02:12.23 -13:02:39.1: ref_mag=14.94 +/- 0.13 new_mean_mag=14.7358 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:24:20.60 -12:47:57.7: 15.11 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:24:20.60 -12:47:57.7: 15.14 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.14
Forced photometry filter REJECTED candidate at 22:24:20.60 -12:47:57.7: ref_mag=15.13 +/- 0.14 new_mean_mag=14.6378 delta=0.49 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:37:36.99 -12:48:40.2: 14.69 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:37:36.99 -12:48:40.2: 14.72 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.11
Forced photometry filter REJECTED candidate at 22:37:36.99 -12:48:40.2: ref_mag=14.70 +/- 0.11 new_mean_mag=14.6681 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:48.19 -13:19:44.9: 14.98 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:48.19 -13:19:44.9: 15.26 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.14
Forced photometry filter REJECTED candidate at 22:23:48.19 -13:19:44.9: ref_mag=15.08 +/- 0.14 new_mean_mag=14.7338 delta=0.35 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:48.09 -09:35:36.4: 14.92 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:48.09 -09:35:36.4: 14.87 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.13
Forced photometry filter REJECTED candidate at 22:42:48.09 -09:35:36.4: ref_mag=14.90 +/- 0.13 new_mean_mag=14.7874 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:11.08 -13:31:12.2: 14.98 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:11.08 -13:31:12.2: 15.10 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.16
Forced photometry filter REJECTED candidate at 22:39:11.08 -13:31:12.2: ref_mag=15.03 +/- 0.16 new_mean_mag=14.7741 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:48.98 -13:32:19.2: 14.69 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:48.98 -13:32:19.2: 14.68 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.12
Forced photometry filter REJECTED candidate at 22:42:48.98 -13:32:19.2: ref_mag=14.69 +/- 0.12 new_mean_mag=14.7530 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:41.26 -10:57:00.2: 15.17 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:41.26 -10:57:00.2: 14.98 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.15
Forced photometry filter REJECTED candidate at 22:42:41.26 -10:57:00.2: ref_mag=15.05 +/- 0.15 new_mean_mag=14.7992 delta=0.25 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:27:11.11 -14:11:08.1: 15.20 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:32:30.62 -14:05:20.3: 15.19 +/- 0.25 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:00.78 -11:08:40.9: 15.05 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:32:30.62 -14:05:20.3: 15.02 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:03:33.66 -12:21:11.3: 15.03 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.16
Forced photometry filter REJECTED candidate at 22:32:30.62 -14:05:20.3: ref_mag=15.09 +/- 0.16 new_mean_mag=14.7985 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:27:11.11 -14:11:08.1: 15.06 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.16
Forced photometry filter REJECTED candidate at 22:27:11.11 -14:11:08.1: ref_mag=15.13 +/- 0.16 new_mean_mag=14.8191 delta=0.31 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:00.78 -11:08:40.9: 15.06 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.13
Forced photometry filter REJECTED candidate at 22:36:00.78 -11:08:40.9: ref_mag=15.05 +/- 0.13 new_mean_mag=14.7652 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:30:57.69 -12:43:32.7: 15.13 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:30:57.69 -12:43:32.7: 15.26 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:03:33.66 -12:21:11.3: 15.12 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.15
Forced photometry reference-image weighted average: 15.07 +/- 0.13
Forced photometry filter REJECTED candidate at 22:30:57.69 -12:43:32.7: ref_mag=15.18 +/- 0.15 new_mean_mag=14.6341 delta=0.55 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:03:33.66 -12:21:11.3: ref_mag=15.07 +/- 0.13 new_mean_mag=14.7969 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:52.19 -10:59:48.7: 14.95 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:13.07 -13:57:06.9: 15.12 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:18:13.94 -11:57:32.0: 15.39 +/- 0.26 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:18:13.94 -11:57:32.0: 15.10 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:13.07 -13:57:06.9: 14.94 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.14
Forced photometry reference-image weighted average: 15.20 +/- 0.15
Forced photometry filter REJECTED candidate at 22:18:13.94 -11:57:32.0: ref_mag=15.20 +/- 0.15 new_mean_mag=14.7976 delta=0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:13.07 -13:57:06.9: ref_mag=15.01 +/- 0.14 new_mean_mag=14.8626 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:52.19 -10:59:48.7: 15.18 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.15
Forced photometry filter REJECTED candidate at 22:41:52.19 -10:59:48.7: ref_mag=15.04 +/- 0.15 new_mean_mag=14.7742 delta=0.26 (need > 0.90)
Adding exclusion_list_local.txt__out52758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53392.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 10s
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Considering the candidate 52606_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52606_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 52608_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52608_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 52610_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52610_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 52615_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52615_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 52618_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52618_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 52620_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52620_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 52634_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52634_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
**** FOUND 22:01:43.14 -11:59:43.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52695_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 52695_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
**** FOUND 22:15:18.50 -13:18:37.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52758_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 52758_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 52849_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 52849_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 52938_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 52938_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 52968_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 52968_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 53209_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 53209_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 53245_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53245_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
**** FOUND 22:14:17.86 -12:38:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53259_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 53259_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 53296_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53296_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53314_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53314_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53324_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53324_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53339_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53339_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53359_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 53359_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 53392_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
Preparing report for the candidate 53392_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
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Considering the candidate 53397_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53397_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53401_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53401_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53420_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53420_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53424_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53424_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53439_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53439_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53440_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53440_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53444_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53444_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53456_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53456_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53458_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53458_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53464_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53464_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53482_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53482_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53490_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53490_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53492_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53492_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53502_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53502_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53503_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53503_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53506_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53506_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53509_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53509_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53524_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53524_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53550_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53550_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53555_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53555_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53562_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53562_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53564_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53564_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53572_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53572_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53585_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53585_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 53602_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 53602_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
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Considering the candidate 12218_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261
The candidate 12218_fd_Aqr-04-Q2b1x1_2026-09-18_00-45-18_20.00sec_0.00C_LIGHT_0261 did not pass the final checks
