This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG
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 07 18.3265 2461239.8265 11.13 21:38:28.20 -10:56:53.4
42.93076 -41.95392 galactic Cap Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.306 Unitas 0 -0 0 11.1 0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:38:28.20 -10:56:53.4: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:38:28.20 -10:56:53.4: 15.40 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3265* 21 38 28.20 -10 56 53.4 11.1 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.8265,11.13,0.05,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
VARIABLE_NAME 20260718.3265 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3265 2461239.8265 11.81 21:37:35.44 -07:13:47.0
47.13679 -40.00546 galactic Aqr Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.389 Industria 0 0 0 12.0 0 0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:37:35.44 -07:13:47.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:37:35.44 -07:13:47.0: 15.47 +/- 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,2461239.8265,11.81,0.05,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 20260718.3265 11.81CV 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 07 18.3265 2461239.8265 13.07 21:34:17.05 -11:07:54.5
42.09690 -41.11782 galactic Cap Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.38 Leda -0 0 0 13.2 -0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:34:17.05 -11:07:54.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:34:17.05 -11:07:54.5: 15.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3265* 21 34 17.05 -11 07 54.5 13.1 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.8265,13.07,0.05,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 20260718.3265 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3265 2461239.8265 13.19 21:05:51.90 -05:59:09.8
43.74414 -32.51133 galactic Aqr Second-epoch detections are separated by 1.0" 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.490 Veritas -0 0 0 13.2 -0 -0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:05:51.90 -05:59:09.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:05:51.90 -05:59:09.8: 15.54 +/- 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,2461239.8265,13.19,0.05,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 20260718.3265 13.19CV 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 07 18.3265 2461239.8265 13.57 21:33:01.92 -12:08:53.7
40.70401 -41.28789 galactic Cap Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.558 Carmen 1 -0 1 13.6 0 0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:33:01.92 -12:08:53.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:33:01.92 -12:08:53.7: 15.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.3265* 21 33 01.92 -12 08 53.7 13.6 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.8265,13.57,0.05,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 20260718.3265 13.57CV 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 07 18.3265 2461239.8265 13.86 21:14:39.60 -13:45:44.9
36.37416 -37.89409 galactic Aqr Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1860 Barbarossa -0 1 1 14.1 0 0
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:14:39.60 -13:45:44.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:14:39.60 -13:45:44.9: 15.60 +/- 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,2461239.8265,13.86,0.05,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 20260718.3265 13.86CV 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 07 18.3265 2461239.8265 11.60 21:02:32.86 -06:36:22.4
42.63649 -32.07837 galactic Aqr Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 3" VX Aqr
Type: M
# Max. Min./Amp. JD0 Period
9.900 V 14.600 V 2452803.00000 185.700000000000
The object was not found in astcheck.
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:02:32.86 -06:36:22.4: 13.97 +/- 0.09 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:02:32.86 -06:36:22.4: 13.87 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VX Aqr,2461239.8265,11.60,0.05,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
VX Aqr 20260718.3265 11.60CV 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: 2461209.88849102 18.06.2026 09:19:15.624 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
First image: 2461209.88849102 18.06.2026 09:19:15.624 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Last image: 2461239.82678513 18.07.2026 07:50:24.235 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.83
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 6519
Objects passed selection criteria: 6516
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6297.75
Average stars matched: 6233.25 (98.9758 %)
Memory usage VmPeak: 116740 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 06:40:20 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: 2461209.88849102 18.06.2026 09:19:15.624 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
First image: 2461209.88849102 18.06.2026 09:19:15.624 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Last image: 2461239.82678513 18.07.2026 07:50:24.235 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 63
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 24 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 44902
Objects passed selection criteria: 44798
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: 43405
Average stars matched: 41914.8 (96.5666 %)
Memory usage VmPeak: 149876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 06:43:10 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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461239.82628435
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits exists and is non-empty
Saving wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits to local_wcs_cache/
'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits'
wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits exists and is non-empty
Saving wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits to local_wcs_cache/
'wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits'
wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits'
wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Image size: 937.2'x624.3' 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: 21:25:43.151 -09:59:41.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Image size: 937.1'x624.2' 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: 21:25:43.210 -09:59:59.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:43.151 -09:59:41.00
Second-epoch image center 21:25:43.210 -09:59:59.60
Angular distance between the image centers 0.0052 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Image size: 937.1'x624.2' 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: 21:25:41.081 -09:59:28.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:43.151 -09:59:41.00
Second-epoch image center 21:25:41.081 -09:59:28.60
Angular distance between the image centers 0.0092 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 21:25:43.210 -09:59:59.60
Second-epoch second image center 21:25:41.081 -09:59:28.60
Angular distance between the image centers 0.01227 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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits &> /tmp/tmp.CBxkIaWjm3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits &> /tmp/tmp.6v58Rqp8q9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits &> /tmp/tmp.I0E69GpyIy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits &> /tmp/tmp.3SHnj14VZ8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat
The reference image (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits) and catalog (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat) found
'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 8801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3911 to 329.4899 deg, Dec -15.2504 to -4.7002 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 313.3911 to 329.4899 deg, Dec -15.2504 to -4.7002 deg
Loaded 6720 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): 5462 out of 5621 total matches.
Matched with Tycho-2 5621 out of 8801 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.686550
a=0.000000 b=1.000000 c=22.686550
From vast_summary.log: estimated ref. image limiting mag.: -7.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3911 to 329.4899 deg, Dec -15.2504 to -4.7002 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 313.3911 to 329.4899 deg, Dec -15.2504 to -4.7002 deg
Loaded 6720 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): 5462 out of 5621 total matches.
Matched with Tycho-2 5621 out of 8801 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits (aperture=6.3)
Read 8277 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3910 to 329.4895 deg, Dec -15.2672 to -4.6985 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 313.3910 to 329.4895 deg, Dec -15.2672 to -4.6985 deg
Loaded 6737 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): 5303 out of 5479 total matches.
Matched with Tycho-2 5479 out of 8277 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
2.3 pix Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
2.2 pix fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
2.2 pix fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
2.3 pix wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
2.3 pix wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Limiting magnitude estimates:
14.9 mag. Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
14.8 mag. Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
14.7 mag. fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
14.7 mag. fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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
############ /tmp/tmp.CBxkIaWjm3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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=508, bad_region=1803, passed=8801
Got 8801 stars (including 6562 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 8801 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 7122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 7122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 7122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits N_match=947 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.433 sigma_q4_arcsec=0.379 n_q1=328 n_q2=184 n_q3=286 n_q4=149 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits -region wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6v58Rqp8q9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.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-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.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=545, bad_region=1756, passed=8277
Got 8277 stars (including 6072 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 8277 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 6658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 6656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 6656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits N_match=949 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.441 sigma_q3_arcsec=0.506 sigma_q4_arcsec=0.389 n_q1=330 n_q2=182 n_q3=280 n_q4=157 worst_quadrant_to_overall_ratio=1.194
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits -region wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.I0E69GpyIy (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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.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=420, bad_region=1391, passed=7275
Got 7275 stars (including 5523 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 7275 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits N_match=949 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.454 sigma_q4_arcsec=0.388 n_q1=330 n_q2=180 n_q3=288 n_q4=151 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3SHnj14VZ8 (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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.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=438, bad_region=1426, passed=7324
Got 7324 stars (including 5524 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat
util/solve_plate_with_UCAC5 got 7324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 5991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits N_match=949 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.369 sigma_q2_arcsec=0.453 sigma_q3_arcsec=0.478 sigma_q4_arcsec=0.485 n_q1=327 n_q2=184 n_q3=289 n_q4=149 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits sigma_overall=0.374 worst_q_ratio=1.158
ref2=Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits sigma_overall=0.424 worst_q_ratio=1.194
new1=fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits sigma_overall=0.405 worst_q_ratio=1.120
new2=fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits sigma_overall=0.438 worst_q_ratio=1.107
reference average sigma_overall=0.399 worst_q_ratio=1.176
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386_astrometric_residuals.png (947 matched stars from wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387_astrometric_residuals.png (949 matched stars from wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294_astrometric_residuals.png (949 matched stars from wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295_astrometric_residuals.png (949 matched stars from wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits'
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits'
Preparing the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:02:32.82 -06:36:22.1: 13.73 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:37:35.44 -07:13:47.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:38:28.20 -10:56:53.4: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:02:32.82 -06:36:22.1: 13.66 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:37:35.44 -07:13:47.0: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:38:28.20 -10:56:53.4: 15.40 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Forced photometry filter KEPT candidate at 21:02:32.82 -06:36:22.1: ref_mag=13.69 +/- 0.05 new_mean_mag=11.3767 delta=2.31 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20215.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20213_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
Preparing report for the candidate 20213_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20214_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 20214_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
**** FOUND 21:02:32.82 -06:36:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.252 6910257102549377792 315.63617454480 -06.60588473130 11.0174 9.3042 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20215_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
Preparing report for the candidate 20215_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aqr-03-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 ####
21:38:28.20 -10:56:53.4
21:37:35.44 -07:13:47.0
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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits exists and is non-empty
wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits exists and is non-empty
wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits exists and is non-empty
wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Image size: 937.2'x624.3' 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: 21:25:43.151 -09:59:41.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Image size: 937.1'x624.2' 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: 21:25:43.210 -09:59:59.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:43.151 -09:59:41.00
Second-epoch image center 21:25:43.210 -09:59:59.60
Angular distance between the image centers 0.0052 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Image size: 937.1'x624.2' 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: 21:25:41.081 -09:59:28.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:43.151 -09:59:41.00
Second-epoch image center 21:25:41.081 -09:59:28.60
Angular distance between the image centers 0.0092 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 21:25:43.210 -09:59:59.60
Second-epoch second image center 21:25:41.081 -09:59:28.60
Angular distance between the image centers 0.01227 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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits &> /tmp/tmp.XW4hqZBczi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits &> /tmp/tmp.VlQZVumTLD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits &> /tmp/tmp.MJeCB0ILB0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits &> /tmp/tmp.JcBE4cutYh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits and wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat
The reference image (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits) and catalog (wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat) found
'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 52953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3814 to 329.5422 deg, Dec -15.2623 to -4.6772 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 313.3814 to 329.5422 deg, Dec -15.2623 to -4.6772 deg
Loaded 6763 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): 5434 out of 5979 total matches.
Matched with Tycho-2 5979 out of 52953 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.550600
a=0.000000 b=1.000000 c=22.550600
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 52953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3814 to 329.5422 deg, Dec -15.2623 to -4.6772 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 313.3814 to 329.5422 deg, Dec -15.2623 to -4.6772 deg
Loaded 6763 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): 5434 out of 5979 total matches.
Matched with Tycho-2 5979 out of 52953 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits (aperture=4.9)
Read 54251 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3546 to 329.5111 deg, Dec -15.2744 to -4.6775 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 313.3546 to 329.5111 deg, Dec -15.2744 to -4.6775 deg
Loaded 6777 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): 5375 out of 5982 total matches.
Matched with Tycho-2 5982 out of 54251 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits -> calib.txt_param_ref_wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
2.1 pix Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
2.1 pix fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
2.1 pix fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
2.3 pix wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
2.1 pix wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Limiting magnitude estimates:
15.0 mag. Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
15.0 mag. Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
14.9 mag. fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
14.9 mag. fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.2 (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.XW4hqZBczi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.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=13, blended=2556, bad_region=7638, passed=52940
Got 52940 stars (including 43074 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 52940 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 45870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 45869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 45869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits N_match=945 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.407 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.407 n_q1=323 n_q2=185 n_q3=276 n_q4=161 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits -region wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VlQZVumTLD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.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-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits' -> 'wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
Checking if the catalog wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits
WCS catalog name: wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.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=20, blended=2698, bad_region=8258, passed=54231
Got 54231 stars (including 43608 good ones) from the SExtractor catalog wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 54231 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 46599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 46598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 46598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 948 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits N_match=948 sigma_overall_arcsec=0.435 sigma_q1_arcsec=0.375 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.508 sigma_q4_arcsec=0.412 n_q1=329 n_q2=192 n_q3=266 n_q4=161 worst_quadrant_to_overall_ratio=1.168
The image catalog is written to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits -region wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MJeCB0ILB0 (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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.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=12, blended=2058, bad_region=7266, passed=48889
Got 48889 stars (including 39862 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 48889 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 41930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 41929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 41929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 945 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits N_match=945 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.412 sigma_q3_arcsec=0.460 sigma_q4_arcsec=0.376 n_q1=332 n_q2=187 n_q3=274 n_q4=152 worst_quadrant_to_overall_ratio=1.167
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JcBE4cutYh (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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Checking if the catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
WCS catalog name: wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.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=14, blended=2061, bad_region=7407, passed=49227
Got 49227 stars (including 40004 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat
util/solve_plate_with_UCAC5 got 49227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 42133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 42134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 42133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 947 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits N_match=947 sigma_overall_arcsec=0.436 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.467 sigma_q4_arcsec=0.466 n_q1=334 n_q2=189 n_q3=272 n_q4=152 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits -region wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-49-40_20.00sec_5.00C_LIGHT_0294.fits
Saving fully-calibrated image wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.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_2026-07-18_CI_Aqr-03-Q2b1x1_030044_TTUQ2b1x1_3071780_zwFAOlVG/wcs_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295.fits
Preparing the HTML report for the field Aqr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 20:58:55.05 -07:38:35.5: 14.26 +/- 0.11 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:21:36.63 -08:36:44.8: 13.97 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:26:57.40 -07:35:57.9: 14.18 +/- 0.09 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:26:34.69 -12:13:35.8: 14.50 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:33:49.52 -12:13:58.9: 14.63 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:17:19.78 -11:20:04.5: 13.87 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:33:24.16 -13:22:24.1: 14.34 +/- 0.12 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:33:18.41 -07:01:40.9: 13.57 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:09:59.81 -09:07:40.0: 14.03 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:12:44.86 -07:05:23.7: 14.14 +/- 0.09 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:33:18.41 -07:01:40.9: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:33:24.16 -13:22:24.1: 14.57 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:12:44.86 -07:05:23.7: 13.92 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:21:36.63 -08:36:44.8: 13.89 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:26:34.69 -12:13:35.8: 14.55 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 20:58:55.05 -07:38:35.5: 14.48 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:09:59.81 -09:07:40.0: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry reference-image weighted average: 14.43 +/- 0.09
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry reference-image weighted average: 14.01 +/- 0.06
Forced photometry reference-image weighted average: 14.53 +/- 0.09
Forced photometry filter REJECTED candidate at 21:33:18.41 -07:01:40.9: ref_mag=13.55 +/- 0.04 new_mean_mag=13.5585 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.35 +/- 0.09
Forced photometry filter REJECTED candidate at 21:33:24.16 -13:22:24.1: ref_mag=14.43 +/- 0.09 new_mean_mag=14.3915 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.05 +/- 0.06
Forced photometry filter REJECTED candidate at 21:21:36.63 -08:36:44.8: ref_mag=13.93 +/- 0.05 new_mean_mag=13.9882 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:12:44.86 -07:05:23.7: ref_mag=14.01 +/- 0.06 new_mean_mag=14.2443 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:26:34.69 -12:13:35.8: ref_mag=14.53 +/- 0.09 new_mean_mag=14.6033 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:58:55.05 -07:38:35.5: ref_mag=14.35 +/- 0.09 new_mean_mag=14.4413 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:09:59.81 -09:07:40.0: ref_mag=14.05 +/- 0.06 new_mean_mag=14.2487 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:17:19.78 -11:20:04.5: 13.97 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:26:57.40 -07:35:57.9: 14.22 +/- 0.09 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:33:49.52 -12:13:58.9: 14.28 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry reference-image weighted average: 14.39 +/- 0.09
Forced photometry reference-image weighted average: 14.20 +/- 0.06
Forced photometry filter REJECTED candidate at 21:17:19.78 -11:20:04.5: ref_mag=13.91 +/- 0.05 new_mean_mag=14.2430 delta=-0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:26:57.40 -07:35:57.9: ref_mag=14.20 +/- 0.06 new_mean_mag=14.4809 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:33:49.52 -12:13:58.9: ref_mag=14.39 +/- 0.09 new_mean_mag=14.4228 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:08:57.12 -08:30:57.3: 12.59 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:06:34.17 -14:01:21.8: 13.14 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:34:17.05 -11:07:54.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 20:58:31.88 -08:51:15.2: 12.99 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:05:51.90 -05:59:09.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:33:01.92 -12:08:53.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:04:35.90 -12:46:23.8: 13.37 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:23:58.32 -13:42:43.4: 13.32 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:09:08.46 -10:48:16.0: 13.85 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:10:07.57 -09:51:52.6: 13.72 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:08:57.12 -08:30:57.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:34:17.05 -11:07:54.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 20:58:31.88 -08:51:15.2: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Forced photometry filter REJECTED candidate at 21:08:57.12 -08:30:57.3: ref_mag=12.62 +/- 0.02 new_mean_mag=12.8539 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:06:34.17 -14:01:21.8: 13.18 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 20:58:31.88 -08:51:15.2: ref_mag=13.04 +/- 0.03 new_mean_mag=12.9660 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:04:35.90 -12:46:23.8: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter REJECTED candidate at 21:06:34.17 -14:01:21.8: ref_mag=13.16 +/- 0.03 new_mean_mag=13.4767 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:33:01.92 -12:08:53.7: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:05:51.90 -05:59:09.8: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:23:58.32 -13:42:43.4: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Forced photometry filter REJECTED candidate at 21:04:35.90 -12:46:23.8: ref_mag=13.41 +/- 0.04 new_mean_mag=13.4615 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter REJECTED candidate at 21:23:58.32 -13:42:43.4: ref_mag=13.32 +/- 0.03 new_mean_mag=13.3648 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:10:07.57 -09:51:52.6: 13.76 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:09:08.46 -10:48:16.0: 13.75 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter REJECTED candidate at 21:10:07.57 -09:51:52.6: ref_mag=13.74 +/- 0.04 new_mean_mag=13.8026 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.80 +/- 0.06
Forced photometry filter REJECTED candidate at 21:09:08.46 -10:48:16.0: ref_mag=13.80 +/- 0.06 new_mean_mag=13.7961 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:06:52.20 -06:41:24.8: 13.63 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:16:15.51 -09:14:44.2: 13.77 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:14:39.60 -13:45:44.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:35:26.54 -12:58:32.1: 13.80 +/- 0.09 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:29:32.19 -12:04:16.0: 14.19 +/- 0.11 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:12:24.05 -08:46:11.3: 14.46 +/- 0.12 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:06:52.20 -06:41:24.8: 13.75 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:14:39.60 -13:45:44.9: 15.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter REJECTED candidate at 21:06:52.20 -06:41:24.8: ref_mag=13.68 +/- 0.04 new_mean_mag=13.8845 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:16:15.51 -09:14:44.2: 13.86 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.06
Forced photometry filter REJECTED candidate at 21:16:15.51 -09:14:44.2: ref_mag=13.81 +/- 0.06 new_mean_mag=13.9445 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:35:26.54 -12:58:32.1: 13.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.06
Forced photometry filter REJECTED candidate at 21:35:26.54 -12:58:32.1: ref_mag=13.78 +/- 0.06 new_mean_mag=13.8197 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 20:59:29.43 -08:13:40.6: 14.06 +/- 0.10 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:29:32.19 -12:04:16.0: 14.01 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.07
Forced photometry filter REJECTED candidate at 21:29:32.19 -12:04:16.0: ref_mag=14.08 +/- 0.07 new_mean_mag=14.0391 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:12:24.05 -08:46:11.3: 14.63 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.10
Forced photometry filter REJECTED candidate at 21:12:24.05 -08:46:11.3: ref_mag=14.52 +/- 0.10 new_mean_mag=14.3729 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 20:59:29.43 -08:13:40.6: 14.37 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.08
Forced photometry filter REJECTED candidate at 20:59:29.43 -08:13:40.6: ref_mag=14.17 +/- 0.08 new_mean_mag=14.3103 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 20:59:40.07 -07:31:58.0: 14.31 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:29:42.49 -11:59:30.4: 15.10 +/- 0.23 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:42:12.27 -11:20:17.4: 14.52 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:02:33.87 -05:47:36.6: 14.65 +/- 0.16 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:33:16.75 -12:45:05.8: 14.73 +/- 0.16 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 20:59:40.07 -07:31:58.0: 14.71 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.10
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:29:42.49 -11:59:30.4: 15.02 +/- 0.21 detection
Forced photometry filter REJECTED candidate at 20:59:40.07 -07:31:58.0: ref_mag=14.45 +/- 0.10 new_mean_mag=14.3140 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 15.06 +/- 0.16
Forced photometry filter REJECTED candidate at 21:29:42.49 -11:59:30.4: ref_mag=15.06 +/- 0.16 new_mean_mag=14.1571 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:42:12.27 -11:20:17.4: 14.37 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.09
Forced photometry filter REJECTED candidate at 21:42:12.27 -11:20:17.4: ref_mag=14.43 +/- 0.09 new_mean_mag=14.1591 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:22:49.04 -05:53:03.1: 14.27 +/- 0.10 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:02:33.87 -05:47:36.6: 14.53 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.11
Forced photometry filter REJECTED candidate at 21:02:33.87 -05:47:36.6: ref_mag=14.59 +/- 0.11 new_mean_mag=14.4369 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:33:16.75 -12:45:05.8: 14.70 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.11
Forced photometry filter REJECTED candidate at 21:33:16.75 -12:45:05.8: ref_mag=14.71 +/- 0.11 new_mean_mag=14.3824 delta=0.33 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:22:49.04 -05:53:03.1: 14.29 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry filter REJECTED candidate at 21:22:49.04 -05:53:03.1: ref_mag=14.28 +/- 0.07 new_mean_mag=14.4400 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:04:02.56 -13:43:48.0: 14.86 +/- 0.20 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:23:09.40 -07:36:58.7: 14.72 +/- 0.16 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:10:15.87 -11:36:20.8: 15.06 +/- 0.22 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:20:11.33 -13:51:51.8: 14.63 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:23:09.40 -07:36:58.7: 14.65 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.11
Forced photometry filter REJECTED candidate at 21:23:09.40 -07:36:58.7: ref_mag=14.68 +/- 0.11 new_mean_mag=14.5620 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:04:02.56 -13:43:48.0: 14.83 +/- 0.20 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:10:15.87 -11:36:20.8: 15.31 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.14
Forced photometry filter REJECTED candidate at 21:04:02.56 -13:43:48.0: ref_mag=14.84 +/- 0.14 new_mean_mag=14.5176 delta=0.33 (need > 0.90)
Forced photometry reference-image weighted average: 15.16 +/- 0.17
Forced photometry filter REJECTED candidate at 21:10:15.87 -11:36:20.8: ref_mag=15.16 +/- 0.17 new_mean_mag=14.6141 delta=0.55 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-18_04-19-15_20.00sec_4.90C_LIGHT_0386.fits at 21:02:32.86 -06:36:22.4: 13.97 +/- 0.09 detection
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:20:11.33 -13:51:51.8: 14.84 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.12
Forced photometry filter REJECTED candidate at 21:20:11.33 -13:51:51.8: ref_mag=14.72 +/- 0.12 new_mean_mag=14.5510 delta=0.17 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q2b1x1_2026-06-22_03-47-39_20.00sec_5.00C_LIGHT_0387.fits at 21:02:32.86 -06:36:22.4: 13.87 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Forced photometry filter KEPT candidate at 21:02:32.86 -06:36:22.4: ref_mag=13.91 +/- 0.06 new_mean_mag=11.5983 delta=2.32 (need > 0.90)
Adding exclusion_list_local.txt__out45051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67232.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: 4s
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Considering the candidate 67117_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67117_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67118_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67118_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67119_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67119_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67125_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67125_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67127_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67127_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67133_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67133_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67136_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67136_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67137_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67137_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67144_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67144_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67148_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67148_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67149_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67149_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67150_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67150_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67152_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67152_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67157_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67157_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
**** FOUND 21:38:28.19 -10:56:53.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 67159_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67159_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
**** FOUND 21:37:35.42 -07:13:47.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 67166_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67166_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67174_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
Preparing report for the candidate 67174_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
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Considering the candidate 67175_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
Preparing report for the candidate 67175_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
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Considering the candidate 67181_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67181_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67189_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
Preparing report for the candidate 67189_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
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Considering the candidate 67220_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67220_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67222_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67222_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67232_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
Preparing report for the candidate 67232_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
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Considering the candidate 67234_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67234_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67240_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67240_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67254_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67254_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67268_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67268_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67291_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67291_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67301_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67301_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67302_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67302_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67308_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67308_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67319_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67319_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67326_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67326_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67336_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67336_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67348_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67348_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67367_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67367_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67371_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67371_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67389_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67389_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
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Considering the candidate 67423_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295
The candidate 67423_fd_Aqr-03-Q2b1x1_2026-07-18_02-50-24_20.00sec_5.00C_LIGHT_0295 did not pass the final checks
