This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX
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 21.3417 2461304.8417 11.40 22:13:14.07 -13:33:07.3
45.07995 -50.71241 galactic Aqr Second-epoch detections are separated by 0.4" and 7.5 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 11.6 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:13:14.07 -13:33:07.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:13:14.07 -13:33:07.3: 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,2461304.8417,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260921.3417 11.40CV 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 21.3417 2461304.8417 12.34 22:28:37.70 -12:15:24.9
49.79904 -53.42256 galactic Aqr Second-epoch detections are separated by 0.3" and 7.5 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 12.6 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:28:37.70 -12:15:24.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:28:37.70 -12:15:24.9: 15.74 +/- 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,2461304.8417,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260921.3417 12.34CV 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 21.3417 2461304.8417 12.84 22:02:48.54 -10:50:24.5
46.95298 -47.20061 galactic Aqr Second-epoch detections are separated by 0.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.78 Diana -0 -0 0 13.1 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:02:48.54 -10:50:24.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:02:48.54 -10:50:24.5: 15.84 +/- 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,2461304.8417,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260921.3417 12.84CV 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 21.3417 2461304.8417 13.39 22:33:06.68 -10:05:57.2
53.84632 -53.25904 galactic Aqr Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.208 Lacrimosa -1 -0 1 13.6 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:33:06.68 -10:05:57.2: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:33:06.68 -10:05:57.2: 15.81 +/- 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,2461304.8417,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260921.3417 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 21.3417 2461304.8417 13.47 22:16:46.72 -11:18:46.7
48.83390 -50.43143 galactic Aqr Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.303 Josephina -0 -0 0 13.7 -0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:46.72 -11:18:46.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:46.72 -11:18:46.7: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461304.8417,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260921.3417 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 21.3417 2461304.8417 14.16 22:25:37.44 -09:24:41.5
53.18569 -51.33216 galactic Aqr Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.846 Lipperta 0 -0 0 14.4 0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:25:37.44 -09:24:41.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:25:37.44 -09:24:41.5: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461304.8417,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260921.3417 14.16CV 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 21.3417 2461304.8417 13.13 22:04:42.44 -08:31:54.8
50.22445 -46.46655 galactic Aqr Second-epoch detections are separated by 0.5" and 7.8 pix
The object was found in VSX 1" CSS_J220442.4-083156
Type: RRAB/BL
# Max. Min./Amp. JD0 Period
13.811 CV Y 0.940 CV 2453705.72920 0.481527900000
The object was not found in astcheck.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:42.44 -08:31:54.8: 14.02 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:42.44 -08:31:54.8: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CSS_J220442.4-083156,2461304.8417,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J220442.4-083156 20260921.3417 13.13CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
First image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461304.84196559 21.09.2026 08:12:15.827 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 5381
Objects passed selection criteria: 5379
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 5102.5
Average stars matched: 4930 (96.6193 %)
Memory usage VmPeak: 232508 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 Mon Sep 21 03:18:53 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
First image: 2461242.93279922 21.07.2026 10:23:03.853 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Last image: 2461304.84196559 21.09.2026 08:12:15.827 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 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): 33119
Objects passed selection criteria: 33047
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 31019.8
Average stars matched: 29918.5 (96.4498 %)
Memory usage VmPeak: 257988 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 Mon Sep 21 03:19:58 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461304.84140752
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.412 -09:59:39.54 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:19.785 -09:59:32.69 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 22:17:19.785 -09:59:32.69
Angular distance between the image centers 0.0836 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:17.193 -09:59:57.15 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 22:17:17.193 -09:59:57.15
Angular distance between the image centers 0.0731 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 22:17:19.785 -09:59:32.69
Second-epoch second image center 22:17:17.193 -09:59:57.15
Angular distance between the image centers 0.01262 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.jnj17MC7Ri
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.kwv0eyoLe7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits &> /tmp/tmp.4eQgk6JHWz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits &> /tmp/tmp.uqGWB900iR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat' -> 'wcsmag.cat'
Read 6925 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Loaded 5569 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4112 out of 4275 total matches.
Matched with Tycho-2 4275 out of 6925 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.666700
a=0.000000 b=1.000000 c=22.666700
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.18
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6925 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8536 to 342.4026 deg, Dec -15.6017 to -4.2140 deg
Loaded 5569 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4112 out of 4275 total matches.
Matched with Tycho-2 4275 out of 6925 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=5.7)
Read 6918 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8535 to 342.3813 deg, Dec -15.6029 to -4.2885 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8535 to 342.3813 deg, Dec -15.6029 to -4.2885 deg
Loaded 5525 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4139 out of 4302 total matches.
Matched with Tycho-2 4302 out of 6918 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=5.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.1 pix Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.4 pix fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
2.4 pix fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Limiting magnitude estimates:
15.2 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.2 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.0 mag. fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
15.0 mag. fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.jnj17MC7Ri (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=496, bad_region=1750, passed=6925
Got 6925 stars (including 4788 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 6925 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4148 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 4126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 5503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4148 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 5503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4126 matched stars entering correct_measured_positions(), 5503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4126 stars left (next iteration limit 4538)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4126 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.337 n_q1=1267 n_q2=739 n_q3=1220 n_q4=900 worst_quadrant_to_overall_ratio=1.321
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.kwv0eyoLe7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=479, bad_region=1750, passed=6918
Got 6918 stars (including 4798 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 6918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4150 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4130 matched stars entering correct_measured_positions(), 4130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4129 matched stars entering correct_measured_positions(), 5496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4149 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4129 matched stars entering correct_measured_positions(), 5496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4129 matched stars entering correct_measured_positions(), 5496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4129 stars left (next iteration limit 4541)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4129 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.317 n_q1=1265 n_q2=760 n_q3=1216 n_q4=888 worst_quadrant_to_overall_ratio=1.291
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4eQgk6JHWz (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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=446, bad_region=1438, passed=6558
Got 6558 stars (including 4794 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 6558 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4158 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4136 matched stars entering correct_measured_positions(), 4136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4136 matched stars entering correct_measured_positions(), 5411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4159 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4136 matched stars entering correct_measured_positions(), 5411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4136 matched stars entering correct_measured_positions(), 5411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4136 stars left (next iteration limit 4549)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4136 robust_rms=7.330 arcsec worst_quadrant_rms=8.632 arcsec
SIP_REFIT: SIP order 3 trial: matched=4136 robust_rms=0.418 arcsec worst_quadrant_rms=0.452 arcsec
SIP_REFIT: SIP order 5 trial: matched=4136 robust_rms=0.356 arcsec worst_quadrant_rms=0.391 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4136 robust_rms_before=0.831 arcsec robust_rms_before_corrected=0.341 arcsec robust_rms_after=0.356 arcsec worst_quadrant_rms_before=0.375 worst_quadrant_rms_after=0.391
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.375 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits N_match=4136 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.383 n_q1=1318 n_q2=828 n_q3=1154 n_q4=836 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.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.uqGWB900iR (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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=461, bad_region=1443, passed=6514
Got 6514 stars (including 4744 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
util/solve_plate_with_UCAC5 got 6514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4111 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4089 matched stars entering correct_measured_positions(), 4089 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4089 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4112 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4089 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4089 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4089 stars left (next iteration limit 4497)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4089 robust_rms=7.380 arcsec worst_quadrant_rms=9.075 arcsec
SIP_REFIT: SIP order 3 trial: matched=4089 robust_rms=0.424 arcsec worst_quadrant_rms=0.452 arcsec
SIP_REFIT: SIP order 5 trial: matched=4089 robust_rms=0.364 arcsec worst_quadrant_rms=0.421 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4089 robust_rms_before=0.843 arcsec robust_rms_before_corrected=0.348 arcsec robust_rms_after=0.364 arcsec worst_quadrant_rms_before=0.373 worst_quadrant_rms_after=0.421
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.373 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits N_match=4089 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.378 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.381 n_q1=1307 n_q2=831 n_q3=1130 n_q4=821 worst_quadrant_to_overall_ratio=1.061
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
Saving the final (post-refit) wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits'
Saving the final (post-refit) wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits sigma_overall=0.361 worst_q_ratio=1.321
ref2=Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits sigma_overall=0.341 worst_q_ratio=1.291
new1=fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits sigma_overall=0.355 worst_q_ratio=1.080
new2=fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits sigma_overall=0.360 worst_q_ratio=1.061
reference average sigma_overall=0.351 worst_q_ratio=1.306
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859_astrometric_residuals.png (4126 matched stars from wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860_astrometric_residuals.png (4129 matched stars from wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249_astrometric_residuals.png (4136 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250_astrometric_residuals.png (4089 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:22:11.91 -09:21:06.4: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:13:14.07 -13:33:07.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:17:21.95 -09:35:11.5: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:23:46.96 -08:09:26.9: 12.05 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:44.70 -08:12:14.8: 12.07 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:15:23.52 -08:39:06.5: 12.13 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:21:13.52 -06:27:18.4: 12.02 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:22:11.91 -09:21:06.4: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:17:21.95 -09:35:11.5: 12.04 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:21:13.52 -06:27:18.4: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter REJECTED candidate at 22:22:11.91 -09:21:06.4: ref_mag=12.00 +/- 0.01 new_mean_mag=11.9351 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:13:14.07 -13:33:07.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:15:23.52 -08:39:06.5: 12.10 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:44.70 -08:12:14.8: 12.05 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 22:17:21.95 -09:35:11.5: ref_mag=12.05 +/- 0.01 new_mean_mag=12.0090 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:21:13.52 -06:27:18.4: ref_mag=12.01 +/- 0.01 new_mean_mag=11.9258 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:23:46.96 -08:09:26.9: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter REJECTED candidate at 22:16:44.70 -08:12:14.8: ref_mag=12.06 +/- 0.01 new_mean_mag=11.9969 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:15:23.52 -08:39:06.5: ref_mag=12.12 +/- 0.01 new_mean_mag=12.0659 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:46.96 -08:09:26.9: ref_mag=12.04 +/- 0.01 new_mean_mag=11.9897 delta=0.05 (need > 0.90)
Adding exclusion_list_local.txt__out20367.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20367_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
Preparing report for the candidate 20367_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20382_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20382_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
**** FOUND 22:04:39.85 -07:11:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20396_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20396_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20400_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20400_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20406_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20406_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20407_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20407_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20409_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20409_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20412_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 20412_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:13:14.07 -13:33:07.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.412 -09:59:39.54 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:19.785 -09:59:32.69 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 22:17:19.785 -09:59:32.69
Angular distance between the image centers 0.0836 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:17.193 -09:59:57.15 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 22:17:17.193 -09:59:57.15
Angular distance between the image centers 0.0731 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 22:17:19.785 -09:59:32.69
Second-epoch second image center 22:17:17.193 -09:59:57.15
Angular distance between the image centers 0.01262 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits &> /tmp/tmp.mGReqeNePb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits &> /tmp/tmp.os9fj2xLae
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits &> /tmp/tmp.QUF2n5lwzt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits &> /tmp/tmp.MgPfo3eOuq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits and wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat' -> 'wcsmag.cat'
Read 44007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Loaded 5591 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4073 out of 4476 total matches.
Matched with Tycho-2 4476 out of 44007 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.559400
a=0.000000 b=1.000000 c=22.559400
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 44007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8306 to 342.4342 deg, Dec -15.6017 to -4.2093 deg
Loaded 5591 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4073 out of 4476 total matches.
Matched with Tycho-2 4476 out of 44007 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (aperture=4.5)
Read 43933 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8257 to 342.4191 deg, Dec -15.6029 to -4.2242 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 325.8257 to 342.4191 deg, Dec -15.6029 to -4.2242 deg
Loaded 5583 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4085 out of 4489 total matches.
Matched with Tycho-2 4489 out of 43933 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
2.0 pix Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Limiting magnitude estimates:
15.4 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
15.3 mag. Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
15.0 mag. fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
15.1 mag. fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (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.mGReqeNePb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1813, bad_region=10057, passed=43988
Got 43988 stars (including 32499 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat
util/solve_plate_with_UCAC5 got 43988 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 4297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 36021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 36021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4297 matched stars entering correct_measured_positions(), 36021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4297 stars left (next iteration limit 4726)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits N_match=4297 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.438 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.314 n_q1=1364 n_q2=840 n_q3=1218 n_q4=875 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.os9fj2xLae (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1714, bad_region=10072, passed=43917
Got 43917 stars (including 32478 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat
util/solve_plate_with_UCAC5 got 43917 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 4295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 35918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4315 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 35918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4295 matched stars entering correct_measured_positions(), 35918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4295 stars left (next iteration limit 4724)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits N_match=4295 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.284 sigma_q4_arcsec=0.303 n_q1=1376 n_q2=836 n_q3=1205 n_q4=878 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits -region wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.QUF2n5lwzt (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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2059, bad_region=5765, passed=34176
Got 34176 stars (including 27280 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 34176 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4310 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 4293 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 29720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4311 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 29720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4293 matched stars entering correct_measured_positions(), 29720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4293 stars left (next iteration limit 4722)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4293 robust_rms=7.081 arcsec worst_quadrant_rms=8.828 arcsec
SIP_REFIT: SIP order 3 trial: matched=4293 robust_rms=0.420 arcsec worst_quadrant_rms=0.449 arcsec
SIP_REFIT: SIP order 5 trial: matched=4293 robust_rms=0.355 arcsec worst_quadrant_rms=0.392 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4293 robust_rms_before=0.834 arcsec robust_rms_before_corrected=0.332 arcsec robust_rms_after=0.355 arcsec worst_quadrant_rms_before=0.378 worst_quadrant_rms_after=0.392
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.378 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits N_match=4293 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.363 n_q1=1411 n_q2=826 n_q3=1245 n_q4=811 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.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.MgPfo3eOuq (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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2086, bad_region=5782, passed=34490
Got 34490 stars (including 27583 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
util/solve_plate_with_UCAC5 got 34490 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4308 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4288 matched stars entering correct_measured_positions(), 4288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4288 matched stars entering correct_measured_positions(), 30020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4308 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4288 matched stars entering correct_measured_positions(), 30020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4288 matched stars entering correct_measured_positions(), 30020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4288 stars left (next iteration limit 4716)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.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=4288 robust_rms=7.123 arcsec worst_quadrant_rms=8.871 arcsec
SIP_REFIT: SIP order 3 trial: matched=4288 robust_rms=0.422 arcsec worst_quadrant_rms=0.448 arcsec
SIP_REFIT: SIP order 5 trial: matched=4288 robust_rms=0.355 arcsec worst_quadrant_rms=0.409 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4288 robust_rms_before=0.840 arcsec robust_rms_before_corrected=0.333 arcsec robust_rms_after=0.355 arcsec worst_quadrant_rms_before=0.358 worst_quadrant_rms_after=0.409
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.358 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits N_match=4288 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.356 n_q1=1413 n_q2=814 n_q3=1246 n_q4=815 worst_quadrant_to_overall_ratio=1.078
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-11-27_20.00sec_-0.00C_LIGHT_0249.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.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_2026-09-21_CI_Aqr-04-Q2b1x1_031630_TTUQ2b1x1_1564224_WTQSrUYX/wcs_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250.fits
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:00.52 -13:36:20.8: 14.11 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:28:49.09 -13:16:17.7: 14.57 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:28:37.70 -12:15:24.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:02:48.54 -10:50:24.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:30:57.52 -10:37:00.9: 13.42 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:33:06.68 -10:05:57.2: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:16:46.72 -11:18:46.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:25:37.44 -09:24:41.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:24.93 -14:04:24.3: 15.08 +/- 0.25 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:28:49.09 -13:16:17.7: 14.78 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:33:06.68 -10:05:57.2: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:16:46.72 -11:18:46.7: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:28:37.70 -12:15:24.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:02:48.54 -10:50:24.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:00.52 -13:36:20.8: 14.13 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:30:57.52 -10:37:00.9: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.10
Forced photometry filter REJECTED candidate at 22:28:49.09 -13:16:17.7: ref_mag=14.66 +/- 0.10 new_mean_mag=14.7169 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 14.12 +/- 0.08
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Forced photometry filter REJECTED candidate at 22:44:00.52 -13:36:20.8: ref_mag=14.12 +/- 0.08 new_mean_mag=14.0577 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:30:57.52 -10:37:00.9: ref_mag=13.40 +/- 0.04 new_mean_mag=13.3712 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:37:44.91 -12:14:47.9: 15.28 +/- 0.26 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:25:37.44 -09:24:41.5: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:24.93 -14:04:24.3: 14.72 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.15
Forced photometry filter REJECTED candidate at 22:42:24.93 -14:04:24.3: ref_mag=14.84 +/- 0.15 new_mean_mag=14.4679 delta=0.37 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:37:44.91 -12:14:47.9: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.16
Forced photometry filter REJECTED candidate at 22:37:44.91 -12:14:47.9: ref_mag=15.11 +/- 0.16 new_mean_mag=14.5904 delta=0.52 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:14.95 -13:19:59.8: 14.58 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:38:54.62 -13:11:42.6: 15.20 +/- 0.26 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:14.88 -13:37:01.2: 14.76 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:25.62 -11:55:10.7: 14.63 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:14.95 -13:19:59.8: 14.89 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.13
Forced photometry filter REJECTED candidate at 22:44:14.95 -13:19:59.8: ref_mag=14.69 +/- 0.13 new_mean_mag=14.4659 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:38:54.62 -13:11:42.6: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.13
Forced photometry filter REJECTED candidate at 22:38:54.62 -13:11:42.6: ref_mag=14.81 +/- 0.13 new_mean_mag=14.5414 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:29:34.01 -14:05:17.1: 14.94 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:14.88 -13:37:01.2: 14.72 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.13
Forced photometry filter REJECTED candidate at 22:41:14.88 -13:37:01.2: ref_mag=14.74 +/- 0.13 new_mean_mag=14.7402 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:25.62 -11:55:10.7: 14.70 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.11
Forced photometry filter REJECTED candidate at 22:41:25.62 -11:55:10.7: ref_mag=14.66 +/- 0.11 new_mean_mag=14.5468 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:29:34.01 -14:05:17.1: 14.90 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.13
Forced photometry filter REJECTED candidate at 22:29:34.01 -14:05:17.1: ref_mag=14.92 +/- 0.13 new_mean_mag=14.6910 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:52.15 -10:12:29.3: 14.89 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:35:41.41 -05:55:07.1: 15.01 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:07.37 -12:11:07.7: 15.60 +/- 0.31 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:39:38.43 -14:05:44.4: 14.96 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:52.15 -10:12:29.3: 15.08 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.13
Forced photometry filter REJECTED candidate at 22:36:52.15 -10:12:29.3: ref_mag=14.97 +/- 0.13 new_mean_mag=14.6511 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:35:41.41 -05:55:07.1: 15.12 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.14
Forced photometry filter REJECTED candidate at 22:35:41.41 -05:55:07.1: ref_mag=15.06 +/- 0.14 new_mean_mag=14.7257 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:42:47.24 -11:15:20.9: 15.13 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:07.37 -12:11:07.7: 15.53 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.56 +/- 0.21
Forced photometry filter REJECTED candidate at 22:31:07.37 -12:11:07.7: ref_mag=15.56 +/- 0.21 new_mean_mag=14.6893 delta=0.87 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:39:38.43 -14:05:44.4: 14.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.14
Forced photometry filter REJECTED candidate at 22:39:38.43 -14:05:44.4: ref_mag=14.86 +/- 0.14 new_mean_mag=14.4706 delta=0.38 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:42:47.24 -11:15:20.9: 14.98 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.15
Forced photometry filter REJECTED candidate at 22:42:47.24 -11:15:20.9: ref_mag=15.04 +/- 0.15 new_mean_mag=14.7155 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:40:32.79 -11:29:33.6: 14.81 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:44:48.16 -10:20:51.7: 15.02 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:38:57.48 -09:05:53.8: 15.05 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:04.27 -12:26:28.4: 15.03 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:40:32.79 -11:29:33.6: 14.84 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.12
Forced photometry filter REJECTED candidate at 22:40:32.79 -11:29:33.6: ref_mag=14.83 +/- 0.12 new_mean_mag=14.8104 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:44:48.16 -10:20:51.7: 14.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.13
Forced photometry filter REJECTED candidate at 22:44:48.16 -10:20:51.7: ref_mag=14.86 +/- 0.13 new_mean_mag=14.8215 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:36:36.04 -13:42:42.4: 14.87 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:38:57.48 -09:05:53.8: 15.36 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.16
Forced photometry filter REJECTED candidate at 22:38:57.48 -09:05:53.8: ref_mag=15.16 +/- 0.16 new_mean_mag=14.7959 delta=0.36 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:04.27 -12:26:28.4: 15.08 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.15
Forced photometry filter REJECTED candidate at 22:36:04.27 -12:26:28.4: ref_mag=15.06 +/- 0.15 new_mean_mag=14.6872 delta=0.37 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:36:36.04 -13:42:42.4: 14.89 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.13
Forced photometry filter REJECTED candidate at 22:36:36.04 -13:42:42.4: ref_mag=14.88 +/- 0.13 new_mean_mag=14.5568 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:41:44.48 -11:55:13.5: 15.22 +/- 0.26 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:25:18.28 -13:21:00.5: 15.31 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:20:33.84 -12:46:56.4: 15.21 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:31:50.71 -12:11:56.4: 15.48 +/- 0.27 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:41:44.48 -11:55:13.5: 14.91 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.15
Forced photometry filter REJECTED candidate at 22:41:44.48 -11:55:13.5: ref_mag=15.02 +/- 0.15 new_mean_mag=14.5593 delta=0.46 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:25:18.28 -13:21:00.5: 15.38 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.17
Forced photometry filter REJECTED candidate at 22:25:18.28 -13:21:00.5: ref_mag=15.35 +/- 0.17 new_mean_mag=14.6864 delta=0.66 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:20:33.84 -12:46:56.4: 15.19 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.14
Forced photometry filter REJECTED candidate at 22:20:33.84 -12:46:56.4: ref_mag=15.20 +/- 0.14 new_mean_mag=14.7249 delta=0.48 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:37:23.76 -06:31:58.0: 15.31 +/- 0.25 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:31:50.71 -12:11:56.4: 14.96 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.14
Forced photometry filter REJECTED candidate at 22:31:50.71 -12:11:56.4: ref_mag=15.10 +/- 0.14 new_mean_mag=14.8014 delta=0.30 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:37:23.76 -06:31:58.0: 14.82 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.14
Forced photometry filter REJECTED candidate at 22:37:23.76 -06:31:58.0: ref_mag=14.96 +/- 0.14 new_mean_mag=14.8449 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:33:29.90 -13:33:34.0: 14.91 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:22:47.16 -12:40:20.1: 15.11 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:11:16.70 -09:19:49.0: 15.22 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:33:29.90 -13:33:34.0: 15.01 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.13
Forced photometry filter REJECTED candidate at 22:33:29.90 -13:33:34.0: ref_mag=14.95 +/- 0.13 new_mean_mag=14.7508 delta=0.20 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:22:47.16 -12:40:20.1: 15.25 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.14
Forced photometry filter REJECTED candidate at 22:22:47.16 -12:40:20.1: ref_mag=15.17 +/- 0.14 new_mean_mag=14.7967 delta=0.38 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:11:16.70 -09:19:49.0: 15.09 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.13
Forced photometry filter REJECTED candidate at 22:11:16.70 -09:19:49.0: ref_mag=15.15 +/- 0.13 new_mean_mag=14.7406 delta=0.41 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-03_20.00sec_-0.00C_LIGHTs_0859.fits at 22:04:42.44 -08:31:54.8: 14.02 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-07-21_05-23-54_20.00sec_-0.00C_LIGHTs_0860.fits at 22:04:42.44 -08:31:54.8: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Forced photometry filter KEPT candidate at 22:04:42.44 -08:31:54.8: ref_mag=14.10 +/- 0.05 new_mean_mag=13.1303 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out18447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53274.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 5s
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Considering the candidate 52597_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 52597_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 52605_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 52605_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 52679_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 52679_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
**** FOUND 22:13:14.07 -13:33:07.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52740_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
Preparing report for the candidate 52740_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
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Considering the candidate 52836_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 52836_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
**** FOUND 22:23:38.16 -07:10:52.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52845_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
Preparing report for the candidate 52845_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
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Considering the candidate 52928_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
Preparing report for the candidate 52928_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
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Considering the candidate 52956_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 52956_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53007_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
Preparing report for the candidate 53007_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
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Considering the candidate 53229_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53229_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
**** FOUND 22:16:57.08 -09:01:06.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53274_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
Preparing report for the candidate 53274_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
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Considering the candidate 53313_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53313_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
**** FOUND 22:14:17.78 -12:38:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53368_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53368_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53393_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53393_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53427_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53427_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53434_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53434_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53441_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53441_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53446_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53446_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53450_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53450_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53485_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53485_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53491_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53491_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53495_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53495_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53498_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53498_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53510_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53510_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53514_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53514_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53516_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53516_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53520_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53520_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53524_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53524_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53544_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53544_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53545_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53545_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53549_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53549_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53565_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53565_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53566_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53566_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53567_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53567_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53574_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53574_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53587_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53587_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 53607_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 53607_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
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Considering the candidate 12218_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250
The candidate 12218_fd_Aqr-04-Q2b1x1_2026-09-21_03-12-15_20.00sec_-0.00C_LIGHT_0250 did not pass the final checks
