This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB
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 27.4040 2461248.9040 12.54 01:36:15.48 +13:57:19.3
139.14111 -47.50084 galactic Psc Second-epoch detections are separated by 0.7" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.101 Helena -1 -1 1 12.8 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:36:15.48 +13:57:19.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:36:15.48 +13:57:19.3: 16.51 +/- 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,2461248.9040,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4040 2461248.9040 12.65 01:44:01.44 +10:51:40.7
143.23377 -49.92618 galactic Psc Second-epoch detections are separated by 1.4" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -1 -0 1 12.6 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:44:01.44 +10:51:40.7: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:44:01.44 +10:51:40.7: 16.48 +/- 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,2461248.9040,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 12.65CV 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 27.4040 2461248.9040 13.08 01:37:11.86 +10:20:00.2
140.96592 -50.92907 galactic Psc Second-epoch detections are separated by 1.0" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste -0 -0 0 13.1 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:37:11.86 +10:20:00.2: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:37:11.86 +10:20:00.2: 16.36 +/- 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,2461248.9040,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 13.08CV 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 27.4040 2461248.9040 13.59 01:33:17.27 +13:52:30.0
138.13469 -47.75759 galactic Psc Second-epoch detections are separated by 0.5" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.212 Medea -1 -1 1 13.9 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:33:17.27 +13:52:30.0: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:33:17.27 +13:52:30.0: 16.44 +/- 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,2461248.9040,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4040 2461248.9040 14.44 01:45:17.24 +12:48:21.6
142.75712 -47.98210 galactic Psc Second-epoch detections are separated by 0.6" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia -1 -0 1 14.4 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:45:17.24 +12:48:21.6: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:45:17.24 +12:48:21.6: 16.50 +/- 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,2461248.9040,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 14.44CV 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 27.4040 2461248.9040 14.59 01:44:25.41 +09:51:35.7
143.88033 -50.84405 galactic Psc Second-epoch detections are separated by 3.5" and 10.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda -0 -1 1 14.7 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:44:25.41 +09:51:35.7: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:44:25.41 +09:51:35.7: 16.41 +/- 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,2461248.9040,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 14.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4040 2461248.9040 14.63 01:27:34.04 +13:09:07.7
136.34553 -48.77637 galactic Psc Second-epoch detections are separated by 3.3" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.517 Edith -0 -0 0 14.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:27:34.04 +13:09:07.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:27:34.04 +13:09:07.7: 16.34 +/- 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,2461248.9040,14.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 14.63CV 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 27.4040 2461248.9040 14.72 01:36:10.49 +13:21:09.9
139.34277 -48.08838 galactic Psc Second-epoch detections are separated by 0.4" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.295 Theresia -1 -0 1 14.9 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:36:10.49 +13:21:09.9: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:36:10.49 +13:21:09.9: 16.50 +/- 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,2461248.9040,14.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4040 14.72CV 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: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Last image: 2461248.90444458 27.07.2026 09:42:14.012 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 35 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): 7811
Objects passed selection criteria: 7803
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 7497
Average stars matched: 6840.5 (91.2432 %)
Memory usage VmPeak: 234396 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 06:22:59 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: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Last image: 2461248.90444458 27.07.2026 09:42:14.012 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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: 21 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): 40244
Objects passed selection criteria: 40164
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 36441
Average stars matched: 34542.5 (94.7902 %)
Memory usage VmPeak: 262752 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 06:26:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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: 2461248.90356412
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits exists and is non-empty
Saving wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits'
wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits exists and is non-empty
Saving wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits'
wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits'
wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits exists and is non-empty
Saving wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.828 +14:00:12.80 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:53.423 +14:00:21.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:53.423 +14:00:21.10
Angular distance between the image centers 0.0550 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:56.720 +13:59:42.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:56.720 +13:59:42.24
Angular distance between the image centers 0.0688 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 01:46:53.423 +14:00:21.10
Second-epoch second image center 01:46:56.720 +13:59:42.24
Angular distance between the image centers 0.01715 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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits &> /tmp/tmp.rlbobxDB9V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits &> /tmp/tmp.0qes9R4jHr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits &> /tmp/tmp.Laf3cP6Ixv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits &> /tmp/tmp.BmQOu6C6j2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9280 deg, Dec +8.6500 to +19.2744 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 18.3971 to 34.9280 deg, Dec 8.6500 to 19.2744 deg
Loaded 4730 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): 3854 out of 4067 total matches.
Matched with Tycho-2 4067 out of 7679 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950000
a=0.000000 b=1.000000 c=22.950000
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9280 deg, Dec +8.6500 to +19.2744 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 18.3971 to 34.9280 deg, Dec 8.6500 to 19.2744 deg
Loaded 4730 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): 3854 out of 4067 total matches.
Matched with Tycho-2 4067 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits (aperture=6.0)
Read 10112 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4179 to 34.9701 deg, Dec +8.5941 to +19.2743 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 18.4179 to 34.9701 deg, Dec 8.5941 to 19.2743 deg
Loaded 4755 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): 3900 out of 4109 total matches.
Matched with Tycho-2 4109 out of 10112 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
2.3 pix Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
2.6 pix fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
2.6 pix fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
2.0 pix wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
2.3 pix wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
15.7 mag. Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
14.9 mag. fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
14.9 mag. fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (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.rlbobxDB9V (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=0, passed=7679
Got 7679 stars (including 7121 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits N_match=969 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.276 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.216 n_q1=215 n_q2=260 n_q3=251 n_q4=243 worst_quadrant_to_overall_ratio=1.236
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.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.0qes9R4jHr (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=639, bad_region=0, passed=10112
Got 10112 stars (including 9456 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 10112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 9930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 9930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 9930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.20"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits (swarp) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits N_match=973 sigma_overall_arcsec=0.206 sigma_q1_arcsec=0.229 sigma_q2_arcsec=0.223 sigma_q3_arcsec=0.207 sigma_q4_arcsec=0.168 n_q1=218 n_q2=266 n_q3=247 n_q4=242 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits -region wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.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.Laf3cP6Ixv (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=318, bad_region=0, passed=6187
Got 6187 stars (including 5861 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat
util/solve_plate_with_UCAC5 got 6187 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 6042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=971 robust_rms=10.080 arcsec
SIP_REFIT: SIP order 3 trial: matched=971 robust_rms=0.334 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=971 robust_rms_before=1.003 arcsec robust_rms_before_corrected=0.246 arcsec robust_rms_after=0.334 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.246 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits N_match=971 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.287 sigma_q3_arcsec=0.219 sigma_q4_arcsec=0.248 n_q1=233 n_q2=254 n_q3=255 n_q4=229 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.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.BmQOu6C6j2 (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=335, bad_region=0, passed=6197
Got 6197 stars (including 5854 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 6197 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 6070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 6069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 6069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=970 robust_rms=10.058 arcsec
SIP_REFIT: SIP order 3 trial: matched=970 robust_rms=0.339 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=970 robust_rms_before=1.004 arcsec robust_rms_before_corrected=0.264 arcsec robust_rms_after=0.339 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.264 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits N_match=970 sigma_overall_arcsec=0.271 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.233 n_q1=234 n_q2=246 n_q3=258 n_q4=232 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits sigma_overall=0.283 worst_q_ratio=1.236
ref2=Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits sigma_overall=0.206 worst_q_ratio=1.111
new1=fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits sigma_overall=0.261 worst_q_ratio=1.101
new2=fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits sigma_overall=0.271 worst_q_ratio=1.128
reference average sigma_overall=0.2445 worst_q_ratio=1.1735
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1_astrometric_residuals.png (969 matched stars from wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2_astrometric_residuals.png (973 matched stars from wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.19 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288_astrometric_residuals.png (971 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289_astrometric_residuals.png (970 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits'
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:39.828 +14:00:12.80 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:53.423 +14:00:21.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:53.423 +14:00:21.10
Angular distance between the image centers 0.0550 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:56.720 +13:59:42.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.828 +14:00:12.80
Second-epoch image center 01:46:56.720 +13:59:42.24
Angular distance between the image centers 0.0688 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 01:46:53.423 +14:00:21.10
Second-epoch second image center 01:46:56.720 +13:59:42.24
Angular distance between the image centers 0.01715 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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits &> /tmp/tmp.zJYTtC22YG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits &> /tmp/tmp.Qha6FiLE8E
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits &> /tmp/tmp.sWfuMSGKO9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits &> /tmp/tmp.CIuBF12clP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9782 deg, Dec +8.6329 to +19.2915 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 18.3971 to 34.9782 deg, Dec 8.6329 to 19.2915 deg
Loaded 4751 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): 3680 out of 4108 total matches.
Matched with Tycho-2 4108 out of 40639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.860200
a=0.000000 b=1.000000 c=22.860200
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3971 to 34.9782 deg, Dec +8.6329 to +19.2915 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 18.3971 to 34.9782 deg, Dec 8.6329 to 19.2915 deg
Loaded 4751 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): 3680 out of 4108 total matches.
Matched with Tycho-2 4108 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits (aperture=4.9)
Read 46104 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4025 to 35.0124 deg, Dec +8.5911 to +19.2851 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 18.4025 to 35.0124 deg, Dec 8.5911 to 19.2851 deg
Loaded 4781 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): 3597 out of 4113 total matches.
Matched with Tycho-2 4113 out of 46104 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits:
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits (aperture=5.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
2.2 pix Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
2.6 pix fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
2.5 pix fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
2.0 pix wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
2.2 pix wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Limiting magnitude estimates:
15.5 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
15.8 mag. Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
14.9 mag. fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
15.0 mag. fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zJYTtC22YG (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits' -> 'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1873, bad_region=4, passed=40626
Got 40626 stars (including 38681 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 40626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 39711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 39708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 39707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits N_match=968 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.278 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.224 n_q1=210 n_q2=268 n_q3=245 n_q4=245 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits -region wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.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.Qha6FiLE8E (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits' -> 'wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2633, bad_region=1, passed=46084
Got 46084 stars (including 43377 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 46084 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.20"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits N_match=972 sigma_overall_arcsec=0.199 sigma_q1_arcsec=0.223 sigma_q2_arcsec=0.210 sigma_q3_arcsec=0.190 sigma_q4_arcsec=0.168 n_q1=209 n_q2=276 n_q3=244 n_q4=243 worst_quadrant_to_overall_ratio=1.122
The image catalog is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits -region wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.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.sWfuMSGKO9 (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1116, bad_region=10, passed=29760
Got 29760 stars (including 28587 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat
util/solve_plate_with_UCAC5 got 29760 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 29009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 29009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 29009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits N_match=969 sigma_overall_arcsec=0.260 sigma_q1_arcsec=0.244 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.215 sigma_q4_arcsec=0.274 n_q1=229 n_q2=248 n_q3=259 n_q4=233 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.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.CIuBF12clP (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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1009, bad_region=16, passed=30215
Got 30215 stars (including 29139 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 30215 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 29593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 29594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 29594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits N_match=970 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.304 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.266 n_q1=232 n_q2=243 n_q3=261 n_q4=234 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits -region wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-40-57_20.00sec_0.00C_LIGHTs_0288.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.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_2026-07-27_CI_Psc-03-Q1b1x1_044426_TTUQ1b1x1_2601351_94aZMYgB/wcs_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289.fits
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:21:10.28 +13:12:02.3: 14.21 +/- 0.07 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:25:44.81 +14:01:18.2: 13.83 +/- 0.05 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:35:39.98 +16:26:59.0: 13.22 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:53:22.82 +12:53:23.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:27:05.29 +15:36:31.9: 12.33 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 02:02:32.67 +08:57:33.7: 14.07 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:35:39.98 +16:26:59.0: 13.25 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:21:10.28 +13:12:02.3: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.01
Forced photometry filter REJECTED candidate at 01:35:39.98 +16:26:59.0: ref_mag=13.24 +/- 0.01 new_mean_mag=13.2347 delta=0.00 (need > 0.90)
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:25:44.81 +14:01:18.2: 13.70 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 01:21:10.28 +13:12:02.3: ref_mag=14.12 +/- 0.04 new_mean_mag=14.1751 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:27:05.29 +15:36:31.9: 12.23 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 01:25:44.81 +14:01:18.2: ref_mag=13.74 +/- 0.03 new_mean_mag=13.8894 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter REJECTED candidate at 01:27:05.29 +15:36:31.9: ref_mag=12.26 +/- 0.01 new_mean_mag=12.4393 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:53:22.82 +12:53:23.6: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 01:53:22.82 +12:53:23.6: ref_mag=12.59 +/- 0.01 new_mean_mag=12.8024 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:43:06.03 +12:34:14.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 02:02:32.67 +08:57:33.7: 13.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter REJECTED candidate at 02:02:32.67 +08:57:33.7: ref_mag=13.87 +/- 0.03 new_mean_mag=14.2338 delta=-0.37 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:37:11.86 +10:20:00.2: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:36:15.48 +13:57:19.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:44:01.44 +10:51:40.7: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:43:06.03 +12:34:14.0: 12.53 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:37:11.86 +10:20:00.2: 16.36 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter REJECTED candidate at 01:43:06.03 +12:34:14.0: ref_mag=12.56 +/- 0.01 new_mean_mag=12.6661 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:33:17.27 +13:52:30.0: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:44:01.44 +10:51:40.7: 16.48 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:37:59.20 +18:28:37.4: 13.54 +/- 0.04 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:36:15.48 +13:57:19.3: 16.51 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:33:17.27 +13:52:30.0: 16.44 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:37:59.20 +18:28:37.4: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter REJECTED candidate at 01:37:59.20 +18:28:37.4: ref_mag=13.50 +/- 0.02 new_mean_mag=13.5588 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 02:08:03.07 +15:46:12.1: 13.98 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:53:09.00 +14:52:23.3: 14.22 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 02:01:36.24 +14:32:26.6: 14.07 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:39:36.46 +14:00:37.1: 14.61 +/- 0.09 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 02:08:03.07 +15:46:12.1: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.04
Forced photometry filter REJECTED candidate at 02:08:03.07 +15:46:12.1: ref_mag=14.06 +/- 0.04 new_mean_mag=14.1025 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:45:17.24 +12:48:21.6: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:53:09.00 +14:52:23.3: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.05
Forced photometry filter REJECTED candidate at 01:53:09.00 +14:52:23.3: ref_mag=14.20 +/- 0.05 new_mean_mag=14.2361 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:44:25.41 +09:51:35.7: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 02:01:36.24 +14:32:26.6: 13.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.03
Forced photometry filter REJECTED candidate at 02:01:36.24 +14:32:26.6: ref_mag=14.00 +/- 0.03 new_mean_mag=14.2239 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:39:36.46 +14:00:37.1: 14.54 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.05
Forced photometry filter REJECTED candidate at 01:39:36.46 +14:00:37.1: ref_mag=14.57 +/- 0.05 new_mean_mag=14.2983 delta=0.27 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:45:17.24 +12:48:21.6: 16.50 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:44:25.41 +09:51:35.7: 16.41 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:34:58.33 +14:22:00.2: 14.32 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:27:34.04 +13:09:07.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_stack1.fits at 01:36:10.49 +13:21:09.9: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:34:58.33 +14:22:00.2: 14.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.05
Forced photometry filter REJECTED candidate at 01:34:58.33 +14:22:00.2: ref_mag=14.32 +/- 0.05 new_mean_mag=14.6543 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:27:34.04 +13:09:07.7: 16.34 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-17_22-10-15_20.00sec_-14.90C_LIGHT_0136_stack2.fits at 01:36:10.49 +13:21:09.9: 16.50 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out56718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57378.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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: 7s
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Considering the candidate 56511_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56511_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56513_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56513_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56514_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56514_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:45:28.87 +17:08:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56515_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56515_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:34:43.15 +18:58:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56518_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56518_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56522_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56522_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56523_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56523_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56524_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56524_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:28:05.36 +18:32:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56525_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56525_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:28:36.30 +14:39:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56682_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56682_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56718_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 56718_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 56747_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56747_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 56754_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 56754_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 56816_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 56816_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 56978_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 56978_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 56992_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 56992_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 57037_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57037_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:39:44.50 +16:26:00.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 57060_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57060_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:48:50.96 +16:23:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57101_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57101_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:44:30.96 +14:02:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57141_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57141_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:43:42.58 +12:53:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57170_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57170_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 02:01:25.81 +17:58:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57195_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57195_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 57202_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57202_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
**** FOUND 01:48:36.56 +10:04:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57219_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57219_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 57240_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57240_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 57271_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57271_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 57305_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 57305_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 57313_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 57313_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 57357_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 57357_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
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Considering the candidate 57361_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 57361_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 57378_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
Preparing report for the candidate 57378_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
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Considering the candidate 31656_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289
The candidate 31656_fd_Psc-03-Q1b1x1_2026-07-27_04-42-14_20.00sec_-0.00C_LIGHTs_0289 did not pass the final checks
