This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD
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 12.2430 2461295.7430 11.18 22:19:42.25 -12:47:30.4
47.30919 -51.76632 galactic Aqr Second-epoch detections are separated by 0.4" and 10.0 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 11.4 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:19:42.25 -12:47:30.4: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:19:42.25 -12:47:30.4: 15.69 +/- 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,2461295.7430,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 11.18CV 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 12.2430 2461295.7430 12.15 22:36:11.90 -12:18:38.6
51.28979 -55.05464 galactic Aqr Second-epoch detections are separated by 0.3" and 10.1 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 12.4 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:11.90 -12:18:38.6: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:11.90 -12:18:38.6: 15.68 +/- 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,2461295.7430,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.2430 2461295.7430 12.70 22:09:47.73 -10:31:58.1
48.59094 -48.55472 galactic Aqr Second-epoch detections are separated by 0.4" and 9.9 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 12.9 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:09:47.73 -10:31:58.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:09:47.73 -10:31:58.1: 15.91 +/- 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,2461295.7430,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.2430 2461295.7430 13.26 22:39:40.04 -09:33:18.6
56.11251 -54.31354 galactic Aqr Second-epoch detections are separated by 0.8" and 10.2 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 13.4 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:40.04 -09:33:18.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:40.04 -09:33:18.6: 15.67 +/- 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,2461295.7430,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 13.26CV 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 12.2430 2461295.7430 13.29 22:23:02.70 -11:03:04.2
50.40511 -51.63742 galactic Aqr Second-epoch detections are separated by 0.2" and 9.9 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 13.5 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:02.70 -11:03:04.2: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:02.70 -11:03:04.2: 15.87 +/- 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,2461295.7430,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.2430 2461295.7430 14.13 22:44:52.22 -09:46:10.8
57.05809 -55.49456 galactic Aqr Second-epoch detections are separated by 1.9" and 10.0 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 14.5 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:52.22 -09:46:10.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:52.22 -09:46:10.8: 15.57 +/- 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,2461295.7430,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.13CV 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 12.2430 2461295.7430 14.07 22:29:08.06 -14:41:55.7
46.22082 -54.67429 galactic Aqr Second-epoch detections are separated by 1.0" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.367 Amicitia -1 -1 1 13.8 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:29:08.06 -14:41:55.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:29:08.06 -14:41:55.7: 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,2461295.7430,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.07CV 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 12.2430 2461295.7430 14.01 22:31:39.04 -08:49:10.3
55.29574 -52.25998 galactic Aqr Second-epoch detections are separated by 0.9" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.846 Lipperta -1 0 1 14.2 0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:39.04 -08:49:10.3: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:39.04 -08:49:10.3: 15.87 +/- 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,2461295.7430,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.01CV 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 12.2430 2461295.7430 14.15 22:16:59.42 -13:52:07.9
45.27590 -51.67023 galactic Aqr Second-epoch detections are separated by 1.2" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1331 Solvejg -0 -1 1 14.3 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:59.42 -13:52:07.9: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:59.42 -13:52:07.9: 15.77 +/- 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,2461295.7430,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.2430 2461295.7430 14.22 21:52:08.59 -13:17:44.3
42.04745 -45.98810 galactic Cap Second-epoch detections are separated by 2.6" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1082 Pirola 1 -1 1 14.2 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:52:08.59 -13:17:44.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:52:08.59 -13:17:44.3: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 12.2430* 21 52 08.59 -13 17 44.3 14.2 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461295.7430,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.2430 2461295.7430 14.46 22:44:59.45 -10:33:25.9
55.92848 -55.95980 galactic Aqr Second-epoch detections are separated by 1.6" and 10.4 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 14.6 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:59.45 -10:33:25.9: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:59.45 -10:33:25.9: 15.45 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.45 +/- 0.33
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,2461295.7430,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.46CV 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 12.2430 2461295.7430 14.76 22:06:11.26 -05:30:55.1
54.16967 -45.17132 galactic Aqr Second-epoch detections are separated by 2.0" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.854 Frostia -1 -0 1 14.6 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:06:11.26 -05:30:55.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:06:11.26 -05:30:55.1: 15.87 +/- 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,2461295.7430,14.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.2430 14.76CV 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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461295.74330376 12.09.2026 05:50:11.445 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 6 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): 7412
Objects passed selection criteria: 7408
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 7134.5
Average stars matched: 6861.5 (96.1735 %)
Memory usage VmPeak: 233420 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 Sat Sep 12 00:57:25 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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461295.74330376 12.09.2026 05:50:11.445 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 45 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): 43979
Objects passed selection criteria: 43853
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 42555.5
Average stars matched: 41163 (96.7278 %)
Memory usage VmPeak: 263796 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 Sat Sep 12 01:00:00 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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: 2461295.74269073
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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Image size: 941.1'x626.7' 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: 22:17:26.596 -10:00:29.38 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 22:17:26.596 -10:00:29.38
Angular distance between the image centers 0.1124 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Image size: 941.1'x626.7' 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: 22:17:29.618 -10:01:08.59 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 22:17:29.618 -10:01:08.59
Angular distance between the image centers 0.1264 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 22:17:26.596 -10:00:29.38
Second-epoch second image center 22:17:29.618 -10:01:08.59
Angular distance between the image centers 0.01650 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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.16JqRRZ56H
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.AnlNed5lTf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits &> /tmp/tmp.t9zTa0CkXn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits &> /tmp/tmp.XiLMIjgyBt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_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 22.673200
a=0.000000 b=1.000000 c=22.673200
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.16
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=5.8)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.1 pix Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.4 pix fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
2.4 pix fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Limiting magnitude estimates:
15.2 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.2 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.1 mag. fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
15.1 mag. fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.0 (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.16JqRRZ56H (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=496, bad_region=0, passed=6925
Got 6925 stars (including 6418 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_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 4341 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6925 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 4341 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4318 stars left (next iteration limit 4749)
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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4318 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.316 sigma_q4_arcsec=0.319 n_q1=1030 n_q2=1223 n_q3=924 n_q4=1141 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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.AnlNed5lTf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=479, bad_region=0, passed=6918
Got 6918 stars (including 6429 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_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 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: 4319 matched stars entering correct_measured_positions(), 4319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4318 matched stars entering correct_measured_positions(), 6918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 4338 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4316 matched stars entering correct_measured_positions(), 6918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4316 matched stars entering correct_measured_positions(), 6918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4316 stars left (next iteration limit 4749)
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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4316 sigma_overall_arcsec=0.331 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.300 n_q1=1033 n_q2=1228 n_q3=924 n_q4=1131 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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.t9zTa0CkXn (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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=531, bad_region=0, passed=7486
Got 7486 stars (including 6944 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 7486 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 4346 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4324 matched stars entering correct_measured_positions(), 4325 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4324 matched stars entering correct_measured_positions(), 7486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 4347 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4325 matched stars entering correct_measured_positions(), 7486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4325 matched stars entering correct_measured_positions(), 7486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4325 stars left (next iteration limit 4756)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4325 robust_rms=13.231 arcsec worst_quadrant_rms=14.867 arcsec
SIP_REFIT: SIP order 3 trial: matched=4325 robust_rms=0.388 arcsec worst_quadrant_rms=0.413 arcsec
SIP_REFIT: SIP order 5 trial: matched=4325 robust_rms=0.256 arcsec worst_quadrant_rms=0.266 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4325 robust_rms_before=0.916 arcsec robust_rms_before_corrected=0.277 arcsec robust_rms_after=0.256 arcsec worst_quadrant_rms_before=0.293 worst_quadrant_rms_after=0.266
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.293 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits N_match=4325 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.293 sigma_q2_arcsec=0.304 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.290 n_q1=1045 n_q2=1221 n_q3=932 n_q4=1127 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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.XiLMIjgyBt (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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, bad_region=0, passed=7500
Got 7500 stars (including 6980 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 7500 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 4347 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4325 matched stars entering correct_measured_positions(), 4326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4325 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 4347 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4328 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4327 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4327 stars left (next iteration limit 4757)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4327 robust_rms=13.262 arcsec worst_quadrant_rms=14.935 arcsec
SIP_REFIT: SIP order 3 trial: matched=4327 robust_rms=0.387 arcsec worst_quadrant_rms=0.407 arcsec
SIP_REFIT: SIP order 5 trial: matched=4327 robust_rms=0.253 arcsec worst_quadrant_rms=0.265 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4327 robust_rms_before=0.917 arcsec robust_rms_before_corrected=0.277 arcsec robust_rms_after=0.253 arcsec worst_quadrant_rms_before=0.296 worst_quadrant_rms_after=0.265
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Image size: 941.1'x626.8' 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: 22:17:29.655 -10:01:08.93 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7500 stars ###
'wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/correct_sextractor_wcs_catalog_usingxy2sky2438437.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.917 -> 0.253 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4327 pairs from the initial matching)
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 4142 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4142 pairs (4327 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4142 robust_rms=13.159 arcsec worst_quadrant_rms=14.763 arcsec
SIP_REFIT: SIP order 3 trial: matched=4142 robust_rms=0.383 arcsec worst_quadrant_rms=0.403 arcsec
SIP_REFIT: SIP order 5 trial: matched=4142 robust_rms=0.252 arcsec worst_quadrant_rms=0.263 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4142 robust_rms_before=0.252 arcsec robust_rms_before_corrected=0.252 arcsec robust_rms_after=0.252 arcsec worst_quadrant_rms_before=0.264 worst_quadrant_rms_after=0.263
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Image size: 941.1'x626.8' 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: 22:17:29.655 -10:01:08.93 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7500 stars ###
'wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/correct_sextractor_wcs_catalog_usingxy2sky2462526.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.252 -> 0.252 arcsec)
Accuracy estimation diagnostic: 4142 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4142 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits N_match=4142 sigma_overall_arcsec=0.269 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.290 sigma_q3_arcsec=0.243 sigma_q4_arcsec=0.268 n_q1=997 n_q2=1165 n_q3=896 n_q4=1084 worst_quadrant_to_overall_ratio=1.078
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
Saving the final (post-refit) wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits sigma_overall=0.352 worst_q_ratio=1.115
ref2=Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits sigma_overall=0.331 worst_q_ratio=1.177
new1=fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits sigma_overall=0.288 worst_q_ratio=1.057
new2=fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits sigma_overall=0.269 worst_q_ratio=1.078
reference average sigma_overall=0.3415 worst_q_ratio=1.146
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859_astrometric_residuals.png (4318 matched stars from wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860_astrometric_residuals.png (4316 matched stars from wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224_astrometric_residuals.png (4325 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225_astrometric_residuals.png (4142 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.20 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits'
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:22:11.92 -09:21:06.2: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:05.88 -08:06:07.9: 12.08 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:17:21.97 -09:35:11.3: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:19:42.25 -12:47:30.4: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:46.98 -08:09:26.5: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:21:13.53 -06:27:18.4: 12.02 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:44.65 -08:12:16.6: 12.09 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:17:21.97 -09:35:11.3: 12.04 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:19:42.25 -12:47:30.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:05.88 -08:06:07.9: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:46.98 -08:09:26.5: 12.02 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:21:13.53 -06:27:18.4: 11.99 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:44.65 -08:12:16.6: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:22:11.92 -09:21:06.2: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter REJECTED candidate at 22:17:21.97 -09:35:11.3: ref_mag=12.05 +/- 0.01 new_mean_mag=12.0369 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter REJECTED candidate at 22:04:05.88 -08:06:07.9: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0765 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:13.53 -06:27:18.4: ref_mag=12.01 +/- 0.01 new_mean_mag=11.9813 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:16:44.65 -08:12:16.6: ref_mag=12.08 +/- 0.01 new_mean_mag=12.0922 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:46.98 -08:09:26.5: ref_mag=12.04 +/- 0.01 new_mean_mag=12.0422 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 22:22:11.92 -09:21:06.2: ref_mag=12.00 +/- 0.01 new_mean_mag=11.9976 delta=0.01 (need > 0.90)
Adding exclusion_list_local.txt__out20419.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: 2s
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Considering the candidate 20419_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 20419_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 20425_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20425_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
**** FOUND 22:04:39.84 -07:11:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20431_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20431_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 20432_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20432_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 20437_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20437_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 20438_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20438_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 20440_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20440_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 20442_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 20442_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 05978_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 05978_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
**** FOUND 22:19:54.44 -14:24:07.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 12s
Prepared the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:19:42.25 -12:47:30.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Image size: 941.1'x626.7' 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: 22:17:26.596 -10:00:29.38 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 22:17:26.596 -10:00:29.38
Angular distance between the image centers 0.1124 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Image size: 941.1'x626.8' 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: 22:17:29.655 -10:01:08.93 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 22:17:29.655 -10:01:08.93
Angular distance between the image centers 0.1266 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 22:17:26.596 -10:00:29.38
Second-epoch second image center 22:17:29.655 -10:01:08.93
Angular distance between the image centers 0.01668 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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.MsH1afvJh1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.T9lFupHhhP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits &> /tmp/tmp.vpB98FDBar
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits &> /tmp/tmp.JgJmh6rvOu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_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 22.570300
a=0.000000 b=1.000000 c=22.570300
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=4.6)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.0 pix Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.3 pix fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
2.3 pix fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Limiting magnitude estimates:
15.3 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.3 mag. Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.3 mag. fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
15.3 mag. fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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.MsH1afvJh1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=1813, bad_region=20, passed=43984
Got 43984 stars (including 42059 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 43984 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 4331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4313 matched stars entering correct_measured_positions(), 4313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4313 matched stars entering correct_measured_positions(), 43984 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 4332 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 43984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 43984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4311 stars left (next iteration limit 4744)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4311 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.311 n_q1=1040 n_q2=1219 n_q3=934 n_q4=1118 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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.T9lFupHhhP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1714, bad_region=21, passed=43912
Got 43912 stars (including 42099 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 43912 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 4334 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4315 matched stars entering correct_measured_positions(), 4315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4315 matched stars entering correct_measured_positions(), 43912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 4333 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4314 matched stars entering correct_measured_positions(), 43912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4314 matched stars entering correct_measured_positions(), 43912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4314 stars left (next iteration limit 4746)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4314 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.290 n_q1=1055 n_q2=1210 n_q3=924 n_q4=1125 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q1b1x1_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-Q1b1x1_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.vpB98FDBar (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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1686, bad_region=3, passed=41924
Got 41924 stars (including 40170 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 41924 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 4330 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 4312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 41924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 4332 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 41924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4311 matched stars entering correct_measured_positions(), 41924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4311 stars left (next iteration limit 4742)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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=4311 robust_rms=13.271 arcsec worst_quadrant_rms=14.529 arcsec
SIP_REFIT: SIP order 3 trial: matched=4311 robust_rms=0.384 arcsec worst_quadrant_rms=0.410 arcsec
SIP_REFIT: SIP order 5 trial: matched=4311 robust_rms=0.250 arcsec worst_quadrant_rms=0.264 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4311 robust_rms_before=0.919 arcsec robust_rms_before_corrected=0.273 arcsec robust_rms_after=0.250 arcsec worst_quadrant_rms_before=0.303 worst_quadrant_rms_after=0.264
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 0.919 -> 0.250 arcsec); the image header was NOT rewritten as wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits is a symbolic link
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4311 pairs from the initial matching)
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 4128 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4128 pairs (4311 from the initial matching)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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=4128 robust_rms=13.134 arcsec worst_quadrant_rms=14.412 arcsec
SIP_REFIT: SIP order 3 trial: matched=4128 robust_rms=0.380 arcsec worst_quadrant_rms=0.408 arcsec
SIP_REFIT: SIP order 5 trial: matched=4128 robust_rms=0.250 arcsec worst_quadrant_rms=0.262 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4128 robust_rms_before=0.250 arcsec robust_rms_before_corrected=0.250 arcsec robust_rms_after=0.250 arcsec worst_quadrant_rms_before=0.262 worst_quadrant_rms_after=0.262
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 0.250 -> 0.250 arcsec); the image header was NOT rewritten as wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits is a symbolic link
Accuracy estimation diagnostic: 4128 matched stars entering correct_measured_positions(), 41924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4128 matched stars entering correct_measured_positions(), 41924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits N_match=4128 sigma_overall_arcsec=0.266 sigma_q1_arcsec=0.266 sigma_q2_arcsec=0.287 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.269 n_q1=999 n_q2=1150 n_q3=909 n_q4=1070 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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.JgJmh6rvOu (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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1680, bad_region=5, passed=41752
Got 41752 stars (including 40009 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 41752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 4339 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4322 matched stars entering correct_measured_positions(), 4322 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 41752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 4339 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 41752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4321 matched stars entering correct_measured_positions(), 41752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4321 stars left (next iteration limit 4753)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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=4321 robust_rms=13.436 arcsec worst_quadrant_rms=14.749 arcsec
SIP_REFIT: SIP order 3 trial: matched=4321 robust_rms=0.386 arcsec worst_quadrant_rms=0.407 arcsec
SIP_REFIT: SIP order 5 trial: matched=4321 robust_rms=0.250 arcsec worst_quadrant_rms=0.265 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4321 robust_rms_before=0.251 arcsec robust_rms_before_corrected=0.265 arcsec robust_rms_after=0.250 arcsec worst_quadrant_rms_before=0.264 worst_quadrant_rms_after=0.265
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.264 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits N_match=4321 sigma_overall_arcsec=0.273 sigma_q1_arcsec=0.268 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.227 sigma_q4_arcsec=0.285 n_q1=1053 n_q2=1212 n_q3=944 n_q4=1112 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-49-18_20.00sec_0.00C_LIGHTs_0224.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.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_2026-09-12_CI_Aqr-04-Q1b1x1_005058_TTUQ1b1x1_1225527_OlZKWBFD/wcs_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225.fits
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:46:55.47 -07:49:01.2: 14.33 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:09:47.73 -10:31:58.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:55:33.82 -08:32:42.2: 14.16 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:22:51.22 -08:49:08.5: 14.09 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:34.66 -13:42:40.3: 14.18 +/- 0.09 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:52:44.78 -10:54:21.1: 14.84 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:59:29.27 -09:44:24.6: 14.42 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:00.62 -13:36:21.8: 14.21 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:11.90 -12:18:38.6: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:47:22.57 -07:43:23.5: 12.80 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:00.62 -13:36:21.8: 14.18 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:09:47.73 -10:31:58.1: 15.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.19 +/- 0.08
Forced photometry filter REJECTED candidate at 22:44:00.62 -13:36:21.8: ref_mag=14.19 +/- 0.08 new_mean_mag=14.1571 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:52:44.78 -10:54:21.1: 14.93 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.12
Forced photometry filter REJECTED candidate at 21:52:44.78 -10:54:21.1: ref_mag=14.89 +/- 0.12 new_mean_mag=14.5616 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:55:33.82 -08:32:42.2: 14.03 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:22:51.22 -08:49:08.5: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Forced photometry filter REJECTED candidate at 21:55:33.82 -08:32:42.2: ref_mag=14.09 +/- 0.05 new_mean_mag=14.3797 delta=-0.29 (need > 0.90)
Forced photometry reference-image weighted average: 14.11 +/- 0.05
Forced photometry filter REJECTED candidate at 22:22:51.22 -08:49:08.5: ref_mag=14.11 +/- 0.05 new_mean_mag=14.5989 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:11.90 -12:18:38.6: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:34.66 -13:42:40.3: 14.31 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:59:29.27 -09:44:24.6: 14.32 +/- 0.09 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:46:55.47 -07:49:01.2: 14.37 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.07
Forced photometry filter REJECTED candidate at 22:04:34.66 -13:42:40.3: ref_mag=14.24 +/- 0.07 new_mean_mag=14.5691 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:47:22.57 -07:43:23.5: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.07
Forced photometry reference-image weighted average: 14.35 +/- 0.07
Forced photometry filter REJECTED candidate at 21:46:55.47 -07:49:01.2: ref_mag=14.35 +/- 0.07 new_mean_mag=14.2994 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:59:29.27 -09:44:24.6: ref_mag=14.37 +/- 0.07 new_mean_mag=14.4955 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 21:47:22.57 -07:43:23.5: ref_mag=12.82 +/- 0.02 new_mean_mag=12.8658 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:40.04 -09:33:18.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:02.70 -11:03:04.2: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:12.09 -10:38:11.1: 13.79 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:52:25.00 -12:31:10.7: 14.02 +/- 0.09 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:39.04 -08:49:10.3: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:52.22 -09:46:10.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:29:08.06 -14:41:55.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:47:21.24 -11:55:54.8: 14.57 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:40.04 -09:33:18.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:12.09 -10:38:11.1: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry filter REJECTED candidate at 22:04:12.09 -10:38:11.1: ref_mag=13.80 +/- 0.04 new_mean_mag=13.8097 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:02.70 -11:03:04.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:52:25.00 -12:31:10.7: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Forced photometry filter REJECTED candidate at 21:52:25.00 -12:31:10.7: ref_mag=13.99 +/- 0.06 new_mean_mag=13.9778 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:39.04 -08:49:10.3: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:52.22 -09:46:10.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:29:08.06 -14:41:55.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:47:21.24 -11:55:54.8: 14.47 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.10
Forced photometry filter REJECTED candidate at 22:47:21.24 -11:55:54.8: ref_mag=14.51 +/- 0.10 new_mean_mag=14.2332 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:59.42 -13:52:07.9: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:52:08.59 -13:17:44.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:54:24.48 -14:06:37.6: 14.74 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:52:08.59 -13:17:44.3: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:59.42 -13:52:07.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:54:24.48 -14:06:37.6: 15.04 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.14
Forced photometry filter REJECTED candidate at 21:54:24.48 -14:06:37.6: ref_mag=14.85 +/- 0.14 new_mean_mag=14.5284 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:00:32.24 -04:46:05.8: 14.46 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:00:32.24 -04:46:05.8: 14.48 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.08
Forced photometry filter REJECTED candidate at 22:00:32.24 -04:46:05.8: ref_mag=14.47 +/- 0.08 new_mean_mag=14.3929 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:50.29 -13:11:14.0: 14.86 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:50.29 -13:11:14.0: 14.58 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.12
Forced photometry filter REJECTED candidate at 22:41:50.29 -13:11:14.0: ref_mag=14.69 +/- 0.12 new_mean_mag=14.5509 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:59.45 -10:33:25.9: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:59.45 -10:33:25.9: 15.45 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.45 +/- 0.33
Forced photometry filter KEPT candidate at 22:44:59.45 -10:33:25.9: ref_mag=15.45 +/- 0.33 new_mean_mag=14.4526 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:45:42.51 -05:22:09.7: 14.62 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:45:42.51 -05:22:09.7: 14.65 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Forced photometry filter REJECTED candidate at 22:45:42.51 -05:22:09.7: ref_mag=14.64 +/- 0.11 new_mean_mag=14.6191 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:55:28.29 -07:59:42.8: 14.99 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:47:46.96 -09:49:26.8: 14.78 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:44.16 -14:21:36.7: 14.79 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:55:28.29 -07:59:42.8: 15.00 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:44.16 -14:21:36.7: 14.47 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:47:46.96 -09:49:26.8: 14.86 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.11
Forced photometry reference-image weighted average: 15.00 +/- 0.12
Forced photometry reference-image weighted average: 14.82 +/- 0.12
Forced photometry filter REJECTED candidate at 22:36:44.16 -14:21:36.7: ref_mag=14.59 +/- 0.11 new_mean_mag=14.7030 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:55:28.29 -07:59:42.8: ref_mag=15.00 +/- 0.12 new_mean_mag=14.6617 delta=0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:47:46.96 -09:49:26.8: ref_mag=14.82 +/- 0.12 new_mean_mag=14.5235 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:49:57.04 -10:25:31.8: 14.63 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:34:40.84 -12:13:09.1: 14.91 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:49:57.04 -10:25:31.8: 14.63 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.10
Forced photometry filter REJECTED candidate at 21:49:57.04 -10:25:31.8: ref_mag=14.63 +/- 0.10 new_mean_mag=14.5740 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:34:40.84 -12:13:09.1: 15.15 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.14
Forced photometry filter REJECTED candidate at 22:34:40.84 -12:13:09.1: ref_mag=15.01 +/- 0.14 new_mean_mag=14.7338 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:48:00.51 -06:45:14.2: 14.84 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:55:01.58 -04:53:28.8: 14.81 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:24:56.28 -14:32:30.1: 15.01 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:49:20.98 -05:32:12.4: 14.78 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:48:00.51 -06:45:14.2: 14.96 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.12
Forced photometry filter REJECTED candidate at 21:48:00.51 -06:45:14.2: ref_mag=14.89 +/- 0.12 new_mean_mag=14.7223 delta=0.17 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:24:56.28 -14:32:30.1: 15.10 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.14
Forced photometry filter REJECTED candidate at 22:24:56.28 -14:32:30.1: ref_mag=15.05 +/- 0.14 new_mean_mag=14.6671 delta=0.38 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:49:20.98 -05:32:12.4: 15.00 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:25.56 -11:55:10.6: 14.61 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry filter REJECTED candidate at 21:49:20.98 -05:32:12.4: ref_mag=14.87 +/- 0.12 new_mean_mag=14.5172 delta=0.35 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:06:11.26 -05:30:55.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:45:06.43 -11:05:22.3: 14.84 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:55:01.58 -04:53:28.8: 15.11 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.12
Forced photometry filter REJECTED candidate at 21:55:01.58 -04:53:28.8: ref_mag=14.93 +/- 0.12 new_mean_mag=14.6908 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:01:04.86 -12:02:58.9: 14.98 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:25:28.18 -14:16:44.9: 14.95 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:28:20.69 -08:02:30.4: 15.26 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:25.56 -11:55:10.6: 14.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:06:11.26 -05:30:55.1: 15.87 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:41:25.56 -11:55:10.6: ref_mag=14.64 +/- 0.11 new_mean_mag=14.5455 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:45:06.43 -11:05:22.3: 14.87 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.13
Forced photometry filter REJECTED candidate at 22:45:06.43 -11:05:22.3: ref_mag=14.85 +/- 0.13 new_mean_mag=14.7471 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:01:04.86 -12:02:58.9: 15.00 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.12
Forced photometry filter REJECTED candidate at 22:01:04.86 -12:02:58.9: ref_mag=14.99 +/- 0.12 new_mean_mag=14.7773 delta=0.22 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:09:54.77 -14:51:34.0: 14.89 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:25:28.18 -14:16:44.9: 14.79 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 22:25:28.18 -14:16:44.9: ref_mag=14.86 +/- 0.12 new_mean_mag=14.7274 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:28:20.69 -08:02:30.4: 15.03 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:38:54.64 -13:11:43.3: 15.15 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.14
Forced photometry filter REJECTED candidate at 22:28:20.69 -08:02:30.4: ref_mag=15.13 +/- 0.14 new_mean_mag=14.8053 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:45:27.93 -11:51:37.5: 14.87 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:14:09.76 -14:34:34.5: 14.81 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:09:54.77 -14:51:34.0: 15.10 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.14
Forced photometry filter REJECTED candidate at 22:09:54.77 -14:51:34.0: ref_mag=14.98 +/- 0.14 new_mean_mag=14.6714 delta=0.31 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:38:54.64 -13:11:43.3: 14.72 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.14
Forced photometry filter REJECTED candidate at 22:38:54.64 -13:11:43.3: ref_mag=14.85 +/- 0.14 new_mean_mag=14.6671 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:34:17.48 -13:33:14.2: 14.82 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:45:27.93 -11:51:37.5: 15.07 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.16
Forced photometry filter REJECTED candidate at 22:45:27.93 -11:51:37.5: ref_mag=14.95 +/- 0.16 new_mean_mag=14.7116 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:07:01.85 -13:48:56.2: 15.06 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 21:54:31.20 -13:34:46.3: 15.11 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:14:09.76 -14:34:34.5: 14.92 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 22:14:09.76 -14:34:34.5: ref_mag=14.86 +/- 0.12 new_mean_mag=14.6319 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:34:17.48 -13:33:14.2: 14.63 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.11
Forced photometry filter REJECTED candidate at 22:34:17.48 -13:33:14.2: ref_mag=14.71 +/- 0.11 new_mean_mag=14.6095 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:07:01.85 -13:48:56.2: 14.95 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.13
Forced photometry filter REJECTED candidate at 22:07:01.85 -13:48:56.2: ref_mag=15.00 +/- 0.13 new_mean_mag=14.6465 delta=0.35 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 21:54:31.20 -13:34:46.3: 15.09 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.16
Forced photometry filter REJECTED candidate at 21:54:31.20 -13:34:46.3: ref_mag=15.10 +/- 0.16 new_mean_mag=14.7732 delta=0.33 (need > 0.90)
Adding exclusion_list_local.txt__out53420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53747.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: 9s
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Considering the candidate 53362_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53362_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53366_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53366_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53369_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53369_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53371_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53371_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53372_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53372_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53374_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53374_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53376_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53376_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53399_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53399_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
**** FOUND 22:19:42.25 -12:47:30.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53420_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53420_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53449_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53449_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53461_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53461_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53487_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53487_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53496_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53496_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53557_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53557_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53579_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53579_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53582_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53582_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53583_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53583_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53589_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53589_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53611_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53611_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53613_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53613_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53628_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53628_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53657_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53657_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53673_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53673_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53684_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53684_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53690_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53690_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53697_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53697_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53702_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53702_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
**** FOUND 22:14:17.78 -12:38:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53711_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53711_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53718_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53718_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53723_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53723_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53726_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53726_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53728_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53728_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53729_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53729_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53739_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53739_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53740_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53740_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53745_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53745_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53747_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
Preparing report for the candidate 53747_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
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Considering the candidate 53755_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53755_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53757_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53757_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53758_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53758_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53762_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53762_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53773_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53773_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53775_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53775_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53777_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53777_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53782_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53782_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53786_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53786_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53787_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53787_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53793_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53793_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 53816_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 53816_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
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Considering the candidate 12218_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 12218_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
**** FOUND 22:04:39.84 -07:11:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33962_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225
The candidate 33962_fd_Aqr-04-Q1b1x1_2026-09-12_00-50-11_20.00sec_-0.00C_LIGHTs_0225 did not pass the final checks
