This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h
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 08 18.3599 2461270.8599 12.12 01:49:23.03 +17:21:24.3
142.09935 -43.34791 galactic Ari Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.101 Helena -1 -1 1 12.4 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:49:23.03 +17:21:24.3: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:49:23.03 +17:21:24.3: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3600* 01 49 23.03 +17 21 24.3 12.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461270.8599,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 12.12CV 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 08 18.3599 2461270.8599 12.78 01:46:37.80 +10:54:52.3
144.14592 -49.67027 galactic Psc Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.124 Alkeste -0 0 0 12.8 -0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:37.80 +10:54:52.3: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:37.80 +10:54:52.3: 16.02 +/- 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,2461270.8599,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 12.78CV 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 08 18.3599 2461270.8599 13.34 01:42:27.96 +15:29:51.7
140.64166 -45.61208 galactic Psc Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.212 Medea 0 -1 1 13.5 -0 -0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:27.96 +15:29:51.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:27.96 +15:29:51.7: 16.10 +/- 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,2461270.8599,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 18.3599 2461270.8599 14.02 01:54:40.06 +10:28:38.0
147.23146 -49.38805 galactic Psc Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.167 Urda -0 0 0 14.4 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:40.06 +10:28:38.0: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:40.06 +10:28:38.0: 16.05 +/- 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,2461270.8599,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 14.02CV 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 08 18.3599 2461270.8599 14.07 01:47:43.72 +12:11:17.7
143.89881 -48.37856 galactic Ari Second-epoch detections are separated by 0.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1317 Silvretta 0 -1 1 14.6 -0 -0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:47:43.72 +12:11:17.7: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:47:43.72 +12:11:17.7: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3600* 01 47 43.72 +12 11 17.7 14.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461270.8599,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 18.3599 2461270.8599 14.23 01:50:47.32 +15:10:07.8
143.51062 -45.31819 galactic Ari Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.295 Theresia -0 -0 0 14.5 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:47.32 +15:10:07.8: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:50:47.32 +15:10:07.8: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3600* 01 50 47.32 +15 10 07.8 14.2 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461270.8599,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 14.23CV 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 08 18.3599 2461270.8599 14.33 01:54:18.29 +13:45:22.4
145.34393 -46.36173 galactic Ari Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia -0 0 0 14.1 0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:18.29 +13:45:22.4: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:18.29 +13:45:22.4: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3600* 01 54 18.29 +13 45 22.4 14.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461270.8599,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 18.3599 2461270.8599 14.48 01:38:23.61 +14:40:25.1
139.60052 -46.67279 galactic Psc Second-epoch detections are separated by 2.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.517 Edith -0 -1 1 14.4 -0 0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:23.61 +14:40:25.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:38:23.61 +14:40:25.1: 16.10 +/- 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,2461270.8599,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 18.3599 2461270.8599 14.66 01:53:15.11 +12:39:06.4
145.55862 -47.48600 galactic Ari Second-epoch detections are separated by 1.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania -1 -1 1 14.7 -0 -0
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:15.11 +12:39:06.4: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:15.11 +12:39:06.4: 16.16 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3600* 01 53 15.11 +12 39 06.4 14.7 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461270.8599,14.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3599 14.66CV 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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461270.86028172 18.08.2026 08:38:38.341 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6776
Objects passed selection criteria: 6744
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 5393.5
Average stars matched: 4972.75 (92.1989 %)
Memory usage VmPeak: 232736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 18 04:34:45 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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461270.86028172 18.08.2026 08:38:38.341 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 47
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 14 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 37888
Objects passed selection criteria: 37756
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 30713.2
Average stars matched: 28099.5 (91.4898 %)
Memory usage VmPeak: 257244 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 18 04:35:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
SExtractor catalog cache: saved Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.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: 2461270.85960953
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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 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: 01:46:39.869 +14:00:12.31 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-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:40.203 +13:59:57.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:40.203 +13:59:57.83
Angular distance between the image centers 0.0042 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:42.897 +13:59:34.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:42.897 +13:59:34.63
Angular distance between the image centers 0.0161 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 01:46:40.203 +13:59:57.83
Second-epoch second image center 01:46:42.897 +13:59:34.63
Angular distance between the image centers 0.01265 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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.eiXGaDRDmG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.s37f21CEW0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits &> /tmp/tmp.r6TueS7Imf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits &> /tmp/tmp.OpvMw8FFSj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 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 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 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): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 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 22.943700
a=0.000000 b=1.000000 c=22.943700
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
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 18.3962 to 34.9286 deg, Dec +8.6498 to +19.2740 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 18.3962 to 34.9286 deg, Dec 8.6498 to 19.2740 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): 3851 out of 4065 total matches.
Matched with Tycho-2 4065 out of 7679 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=5.9)
Read 6762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4566 to 34.9567 deg, Dec +8.6053 to +19.2739 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 18.4566 to 34.9567 deg, Dec 8.6053 to 19.2739 deg
Loaded 4732 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): 3812 out of 4016 total matches.
Matched with Tycho-2 4016 out of 6762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.0 pix Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.3 pix fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
2.3 pix fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.3 mag. Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.2 mag. fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
15.2 mag. fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
All-image limiting magnitude estimate: 15.2 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.eiXGaDRDmG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=1800, passed=7679
Got 7679 stars (including 5466 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 7679 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 6238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 6238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 6238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4879 stars left (next iteration limit 5366)
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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4879 sigma_overall_arcsec=0.245 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.220 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.211 n_q1=1608 n_q2=884 n_q3=1498 n_q4=889 worst_quadrant_to_overall_ratio=1.322
The image catalog is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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.s37f21CEW0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=519, bad_region=1590, passed=6762
Got 6762 stars (including 4768 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 6762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4664 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 4658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4664 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4658 stars left (next iteration limit 5123)
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-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4658 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.252 n_q1=1483 n_q2=869 n_q3=1437 n_q4=869 worst_quadrant_to_overall_ratio=1.350
The image catalog is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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.r6TueS7Imf (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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=433, bad_region=1531, passed=6876
Got 6876 stars (including 4977 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
util/solve_plate_with_UCAC5 got 6876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 4840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 5660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 5660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 5660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4841 stars left (next iteration limit 5324)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4841 robust_rms=6.948 arcsec worst_quadrant_rms=9.661 arcsec
SIP_REFIT: SIP order 3 trial: matched=4841 robust_rms=0.439 arcsec worst_quadrant_rms=0.580 arcsec
SIP_REFIT: SIP order 5 trial: matched=4841 robust_rms=0.334 arcsec worst_quadrant_rms=0.380 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4841 robust_rms_before=0.967 arcsec robust_rms_before_corrected=0.331 arcsec robust_rms_after=0.334 arcsec worst_quadrant_rms_before=0.358 worst_quadrant_rms_after=0.380
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.358 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits N_match=4841 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.347 n_q1=1501 n_q2=902 n_q3=1492 n_q4=946 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits -region wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.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.OpvMw8FFSj (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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=463, bad_region=1512, passed=6807
Got 6807 stars (including 4903 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
util/solve_plate_with_UCAC5 got 6807 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4778 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4775 matched stars entering correct_measured_positions(), 4775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4775 matched stars entering correct_measured_positions(), 5608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4780 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4776 matched stars entering correct_measured_positions(), 5608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4776 matched stars entering correct_measured_positions(), 5608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4776 stars left (next iteration limit 5252)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4776 robust_rms=6.964 arcsec worst_quadrant_rms=9.215 arcsec
SIP_REFIT: SIP order 3 trial: matched=4776 robust_rms=0.467 arcsec worst_quadrant_rms=0.628 arcsec
SIP_REFIT: SIP order 5 trial: matched=4776 robust_rms=0.362 arcsec worst_quadrant_rms=0.403 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4776 robust_rms_before=1.003 arcsec robust_rms_before_corrected=0.366 arcsec robust_rms_after=0.362 arcsec worst_quadrant_rms_before=0.399 worst_quadrant_rms_after=0.403
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.399 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits N_match=4776 sigma_overall_arcsec=0.366 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.391 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.352 n_q1=1506 n_q2=895 n_q3=1447 n_q4=928 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits -region wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
Saving the final (post-refit) wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.245 worst_q_ratio=1.322
ref2=Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits sigma_overall=0.312 worst_q_ratio=1.350
new1=fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits sigma_overall=0.349 worst_q_ratio=1.065
new2=fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits sigma_overall=0.366 worst_q_ratio=1.156
reference average sigma_overall=0.2785 worst_q_ratio=1.336
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (4879 matched stars from wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.22 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139_astrometric_residuals.png (4658 matched stars from wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400_astrometric_residuals.png (4841 matched stars from wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401_astrometric_residuals.png (4776 matched stars from wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits'
Preparing the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:49:23.03 +17:21:24.3: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:49:23.03 +17:21:24.3: 15.93 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out21068.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21068_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 21068_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:49:23.03 +17:21:24.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
SExtractor catalog cache: saved Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Creating symlink local_wcs_cache/wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Image size: 941.5'x627.0' 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: 01:46:39.869 +14:00:12.31 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-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:40.203 +13:59:57.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:40.203 +13:59:57.83
Angular distance between the image centers 0.0042 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:46:42.897 +13:59:34.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:46:39.869 +14:00:12.31
Second-epoch image center 01:46:42.897 +13:59:34.63
Angular distance between the image centers 0.0161 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 01:46:40.203 +13:59:57.83
Second-epoch second image center 01:46:42.897 +13:59:34.63
Angular distance between the image centers 0.01265 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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.LmusbalDwK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.VbWNJi83wE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits &> /tmp/tmp.A0Lzlvwz3D
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits &> /tmp/tmp.O2r4A8pKbe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat' -> 'wcsmag.cat'
Read 40639 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 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 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 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): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 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 22.837800
a=0.000000 b=1.000000 c=22.837800
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
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 18.3962 to 34.9791 deg, Dec +8.6321 to +19.2912 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 18.3962 to 34.9791 deg, Dec 8.6321 to 19.2912 deg
Loaded 4752 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): 3678 out of 4107 total matches.
Matched with Tycho-2 4107 out of 40639 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=4.7)
Read 38153 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.4016 to 34.9977 deg, Dec +8.5904 to +19.2796 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 18.4016 to 34.9977 deg, Dec 8.5904 to 19.2796 deg
Loaded 4774 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): 3712 out of 4109 total matches.
Matched with Tycho-2 4109 out of 38153 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
1.9 pix Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.2 pix fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
2.1 pix fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Limiting magnitude estimates:
15.6 mag. Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.4 mag. Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.3 mag. fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
15.3 mag. fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (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.LmusbalDwK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1873, bad_region=7665, passed=40632
Got 40632 stars (including 31385 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 40632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 34591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 34591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 34591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4884 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4884 sigma_overall_arcsec=0.239 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.215 sigma_q3_arcsec=0.219 sigma_q4_arcsec=0.202 n_q1=1599 n_q2=913 n_q3=1491 n_q4=881 worst_quadrant_to_overall_ratio=1.292
The image catalog is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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.VbWNJi83wE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1585, bad_region=7065, passed=38140
Got 38140 stars (including 29739 good ones) from the SExtractor catalog wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 38140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 32593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 32593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 32593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4888 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4888 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.266 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.248 n_q1=1608 n_q2=911 n_q3=1499 n_q4=870 worst_quadrant_to_overall_ratio=1.364
The image catalog is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.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.A0Lzlvwz3D (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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1517, bad_region=6575, passed=36194
Got 36194 stars (including 28439 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
util/solve_plate_with_UCAC5 got 36194 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 31272 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 31272 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 31272 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4869 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4869 robust_rms=6.695 arcsec worst_quadrant_rms=9.152 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.428 arcsec worst_quadrant_rms=0.556 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.329 arcsec worst_quadrant_rms=0.372 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=0.936 arcsec robust_rms_before_corrected=0.328 arcsec robust_rms_after=0.329 arcsec worst_quadrant_rms_before=0.359 worst_quadrant_rms_after=0.372
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.359 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits N_match=4869 sigma_overall_arcsec=0.342 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.336 n_q1=1535 n_q2=880 n_q3=1468 n_q4=986 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits -region wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.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.O2r4A8pKbe (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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1545, bad_region=6591, passed=36451
Got 36451 stars (including 28632 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
util/solve_plate_with_UCAC5 got 36451 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 31500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 31500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 31500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4868 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4868 robust_rms=6.753 arcsec worst_quadrant_rms=9.126 arcsec
SIP_REFIT: SIP order 3 trial: matched=4868 robust_rms=0.465 arcsec worst_quadrant_rms=0.630 arcsec
SIP_REFIT: SIP order 5 trial: matched=4868 robust_rms=0.359 arcsec worst_quadrant_rms=0.407 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4868 robust_rms_before=0.972 arcsec robust_rms_before_corrected=0.361 arcsec robust_rms_after=0.359 arcsec worst_quadrant_rms_before=0.391 worst_quadrant_rms_after=0.407
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.391 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits N_match=4868 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.333 n_q1=1541 n_q2=881 n_q3=1469 n_q4=977 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits -region wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.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-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-37-40_20.00sec_-0.00C_LIGHT_0400.fits
Saving fully-calibrated image wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.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_2026-08-18_CI_Psc-03-Q2b1x1_034646_TTUQ2b1x1_383514_o1voG32h/wcs_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401.fits
Preparing the HTML report for the field Psc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:36:05.72 +14:36:54.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:26.57 +12:54:48.8: 14.60 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:42:27.96 +15:29:51.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:39:25.99 +12:43:32.9: 14.81 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:37.80 +10:54:52.3: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:40.06 +10:28:38.0: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:47:43.72 +12:11:17.7: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:04:18.83 +14:33:20.1: 13.47 +/- 0.03 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:43:42.62 +12:53:22.0: 14.17 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:08.47 +16:27:44.7: 14.20 +/- 0.06 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:04:18.83 +14:33:20.1: 13.62 +/- 0.04 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:40.06 +10:28:38.0: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:36:05.72 +14:36:54.2: 12.80 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:25.99 +12:43:32.9: 14.78 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:39:26.57 +12:54:48.8: 14.66 +/- 0.10 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:47:43.72 +12:11:17.7: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:37.80 +10:54:52.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:42:27.96 +15:29:51.7: 16.10 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter REJECTED candidate at 02:04:18.83 +14:33:20.1: ref_mag=13.52 +/- 0.02 new_mean_mag=13.6697 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry reference-image weighted average: 14.62 +/- 0.06
Forced photometry reference-image weighted average: 14.80 +/- 0.07
Forced photometry filter REJECTED candidate at 01:36:05.72 +14:36:54.2: ref_mag=12.83 +/- 0.01 new_mean_mag=13.0844 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:39:26.57 +12:54:48.8: ref_mag=14.62 +/- 0.06 new_mean_mag=14.7730 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:39:25.99 +12:43:32.9: ref_mag=14.80 +/- 0.07 new_mean_mag=14.7334 delta=0.06 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:43:42.62 +12:53:22.0: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry filter REJECTED candidate at 01:43:42.62 +12:53:22.0: ref_mag=14.08 +/- 0.04 new_mean_mag=14.1294 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:08.47 +16:27:44.7: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter REJECTED candidate at 01:53:08.47 +16:27:44.7: ref_mag=14.20 +/- 0.04 new_mean_mag=14.1399 delta=0.06 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:58.23 +14:22:01.8: 14.33 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:50:47.32 +15:10:07.8: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:18.29 +13:45:22.4: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:23.61 +14:40:25.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:32:19.66 +10:29:04.0: 14.96 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:58.23 +14:22:01.8: 14.39 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.06
Forced photometry filter REJECTED candidate at 01:34:58.23 +14:22:01.8: ref_mag=14.35 +/- 0.06 new_mean_mag=14.3703 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:18.29 +13:45:22.4: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:38:23.61 +14:40:25.1: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:50:47.32 +15:10:07.8: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:52.12 +13:46:27.1: 14.63 +/- 0.08 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:32:19.66 +10:29:04.0: 15.29 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.11
Forced photometry filter REJECTED candidate at 01:32:19.66 +10:29:04.0: ref_mag=15.06 +/- 0.11 new_mean_mag=14.8020 delta=0.26 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:52.12 +13:46:27.1: 14.86 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.07
Forced photometry filter REJECTED candidate at 01:45:52.12 +13:46:27.1: ref_mag=14.70 +/- 0.07 new_mean_mag=14.7716 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:15.11 +12:39:06.4: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:20.25 +09:57:21.2: 15.17 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:15.11 +12:39:06.4: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:57:26.87 +17:13:13.7: 14.94 +/- 0.11 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:20.25 +09:57:21.2: 15.53 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.14
Forced photometry filter REJECTED candidate at 01:31:20.25 +09:57:21.2: ref_mag=15.27 +/- 0.14 new_mean_mag=14.9299 delta=0.34 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:57:26.87 +17:13:13.7: 14.98 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.09
Forced photometry filter REJECTED candidate at 01:57:26.87 +17:13:13.7: ref_mag=14.96 +/- 0.09 new_mean_mag=14.8709 delta=0.09 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:30:41.27 +10:14:10.7: 15.17 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:33:40.47 +10:25:22.9: 15.58 +/- 0.23 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:30:41.27 +10:14:10.7: 15.07 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.11
Forced photometry filter REJECTED candidate at 01:30:41.27 +10:14:10.7: ref_mag=15.12 +/- 0.11 new_mean_mag=15.0389 delta=0.08 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:33:40.47 +10:25:22.9: 15.13 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.30 +/- 0.14
Forced photometry filter REJECTED candidate at 01:33:40.47 +10:25:22.9: ref_mag=15.30 +/- 0.14 new_mean_mag=14.9462 delta=0.35 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:47.13 +11:38:27.0: 15.49 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:43.80 +10:08:44.2: 15.16 +/- 0.17 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:47.13 +11:38:27.0: 15.63 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.54 +/- 0.15
Forced photometry filter REJECTED candidate at 01:34:47.13 +11:38:27.0: ref_mag=15.54 +/- 0.15 new_mean_mag=15.0846 delta=0.45 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:43.80 +10:08:44.2: 15.65 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.15
Forced photometry filter REJECTED candidate at 01:28:43.80 +10:08:44.2: ref_mag=15.28 +/- 0.15 new_mean_mag=15.0238 delta=0.25 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:34:15.40 +10:29:40.8: 15.04 +/- 0.14 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:46:37.13 +16:54:27.5: 15.41 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:34:15.40 +10:29:40.8: 14.91 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.10
Forced photometry filter REJECTED candidate at 01:34:15.40 +10:29:40.8: ref_mag=14.97 +/- 0.10 new_mean_mag=15.0012 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:46:37.13 +16:54:27.5: 15.33 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.13
Forced photometry filter REJECTED candidate at 01:46:37.13 +16:54:27.5: ref_mag=15.37 +/- 0.13 new_mean_mag=14.9550 delta=0.42 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:29.13 +10:01:52.5: 15.14 +/- 0.16 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:31:51.38 +12:01:22.2: 15.51 +/- 0.20 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:29.13 +10:01:52.5: 15.23 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.13
Forced photometry filter REJECTED candidate at 01:28:29.13 +10:01:52.5: ref_mag=15.18 +/- 0.13 new_mean_mag=14.8812 delta=0.30 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:31:51.38 +12:01:22.2: 15.57 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.53 +/- 0.16
Forced photometry filter REJECTED candidate at 01:31:51.38 +12:01:22.2: ref_mag=15.53 +/- 0.16 new_mean_mag=15.0655 delta=0.47 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:28:46.90 +10:23:16.8: 15.31 +/- 0.19 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:35:45.98 +10:39:55.2: 15.36 +/- 0.18 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:28:46.90 +10:23:16.8: 15.33 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.14
Forced photometry filter REJECTED candidate at 01:28:46.90 +10:23:16.8: ref_mag=15.32 +/- 0.14 new_mean_mag=15.0887 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:35:45.98 +10:39:55.2: 15.29 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.13
Forced photometry filter REJECTED candidate at 01:35:45.98 +10:39:55.2: ref_mag=15.33 +/- 0.13 new_mean_mag=15.1399 delta=0.19 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:29:39.53 +13:37:18.6: 15.57 +/- 0.22 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:02:47.04 +15:07:57.7: 15.68 +/- 0.23 detection
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:29:39.53 +13:37:18.6: 15.18 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.13
Forced photometry filter REJECTED candidate at 01:29:39.53 +13:37:18.6: ref_mag=15.32 +/- 0.13 new_mean_mag=15.0286 delta=0.29 (need > 0.90)
Forced photometry on wcs_Psc-03-Q2b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:02:47.04 +15:07:57.7: 15.56 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.62 +/- 0.16
Forced photometry filter REJECTED candidate at 02:02:47.04 +15:07:57.7: ref_mag=15.62 +/- 0.16 new_mean_mag=15.1573 delta=0.46 (need > 0.90)
Adding exclusion_list_local.txt__out53007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57739.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 51438_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 51438_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 51445_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 51445_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 51449_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 51449_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 52417_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 52417_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 01:49:23.02 +17:21:24.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53007_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 53007_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 53930_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 53930_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 54551_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 54551_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 54641_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 54641_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 01:39:44.50 +16:26:01.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55133_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 55133_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 55412_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 55412_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 55590_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 55590_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 55596_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 55596_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 56114_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 56114_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 56288_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 56288_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 56423_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 56423_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 56515_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 56515_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 56640_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 56640_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 02:02:43.08 +13:27:55.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 57507_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 57507_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 57682_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 57682_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 57739_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 57739_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 57811_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 57811_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58090_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58090_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58109_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58109_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58148_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58148_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58176_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58176_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58278_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58278_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58279_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58279_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58318_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58318_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58324_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58324_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58350_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58350_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58369_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58369_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58419_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58419_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58467_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58467_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 58504_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 58504_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 29370_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401
The candidate 29370_fd_Psc-03-Q2b1x1_2026-08-18_03-38-38_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
