This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 11.72 02:15:55.14 +12:40:42.5
152.87377 -45.22533 galactic Ari Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.46 Hestia -0 0 0 11.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:55.14 +12:40:42.5: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:55.14 +12:40:42.5: 15.70 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.4472* 02 15 55.14 +12 40 42.5 11.7 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,2461292.9472,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 12.36 01:44:57.58 +10:22:19.0
143.81677 -50.31684 galactic Psc Second-epoch detections are separated by 0.2" and 8.5 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 12.4 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:44:57.58 +10:22:19.0: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:44:57.58 +10:22:19.0: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9472,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 12.87 01:41:27.60 +16:13:23.7
140.02576 -44.98179 galactic Psc Second-epoch detections are separated by 0.7" and 8.2 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 -0 0 13.1 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:41:27.60 +16:13:23.7: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:41:27.60 +16:13:23.7: 15.92 +/- 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,2461292.9472,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 13.73 01:54:39.74 +15:59:39.0
144.36541 -44.23046 galactic Ari Second-epoch detections are separated by 0.7" and 8.2 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 14.0 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:39.74 +15:59:39.0: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:39.74 +15:59:39.0: 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 09 09.4472* 01 54 39.74 +15 59 39.0 13.7 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,2461292.9472,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 13.69 01:54:30.40 +10:04:48.3
147.40354 -49.77124 galactic Psc Second-epoch detections are separated by 0.5" and 8.5 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 14.0 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:54:30.40 +10:04:48.3: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:54:30.40 +10:04:48.3: 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,2461292.9472,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 13.82 01:45:12.99 +15:26:16.3
141.57244 -45.47848 galactic Psc Second-epoch detections are separated by 0.8" and 8.3 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 14.1 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:45:12.99 +15:26:16.3: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:45:12.99 +15:26:16.3: 16.11 +/- 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,2461292.9472,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 13.82 01:38:53.30 +15:12:10.8
139.56510 -46.13065 galactic Psc Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.517 Edith 0 0 0 14.0 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:38:53.30 +15:12:10.8: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:38:53.30 +15:12:10.8: 16.07 +/- 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,2461292.9472,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 14.09 01:53:42.54 +13:48:11.4
145.12371 -46.36802 galactic Ari Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.147 Protogeneia 1 -0 1 13.7 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:42.54 +13:48:11.4: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:42.54 +13:48:11.4: 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!
TCP 2026 09 09.4472* 01 53 42.54 +13 48 11.4 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,2461292.9472,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 14.12 01:53:00.53 +14:57:39.3
144.32786 -45.33753 galactic Ari Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1572 Posnania 0 0 0 14.3 -0 -0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:53:00.53 +14:57:39.3: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:53:00.53 +14:57:39.3: 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 09 09.4472* 01 53 00.53 +14 57 39.3 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,2461292.9472,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 14.12CV 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 09 09.4472 2461292.9472 14.36 02:07:15.84 +10:37:12.1
151.43866 -48.01043 galactic Ari Second-epoch detections are separated by 1.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.401 Ottilia 0 -1 1 14.8 0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:07:15.84 +10:37:12.1: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:07:15.84 +10:37:12.1: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.4472* 02 07 15.84 +10 37 12.1 14.4 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,2461292.9472,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 14.87 02:15:53.31 +18:16:26.7
149.53331 -40.19535 galactic Ari Second-epoch detections are separated by 2.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1146 Biarmia 0 -0 0 15.0 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:53.31 +18:16:26.7: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:53.31 +18:16:26.7: 15.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.4472* 02 15 53.31 +18 16 26.7 14.9 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,2461292.9472,14.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 14.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4472 2461292.9472 14.84 01:15:46.85 +09:26:04.0
132.93108 -52.96405 galactic Psc Second-epoch detections are separated by 3.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2251 Tikhov -2 1 2 15.1 -0 0
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:15:46.85 +09:26:04.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:15:46.85 +09:26:04.0: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9472,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4472 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461292.94763850 09.09.2026 10:44:25.966 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 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): 7558
Objects passed selection criteria: 7554
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7171.25
Average stars matched: 7016 (97.8351 %)
Memory usage VmPeak: 233604 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 05:46:34 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
First image: 2461032.69490819 23.12.2025 04:40:30.068 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Last image: 2461292.94763850 09.09.2026 10:44:25.966 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 114
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 17 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): 41327
Objects passed selection criteria: 41203
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 39581.2
Average stars matched: 38012.8 (96.0373 %)
Memory usage VmPeak: 264836 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 05:47:38 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
SExtractor catalog cache: saved Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.cat to cache
SExtractor catalog cache: saved Psc-03-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.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: 2461292.94674317
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits exists and is non-empty
wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits exists and is non-empty
wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (1st reference image)
verification OK: wcs_Psc-03-Q1b1x1_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-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits (1st new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:31.396 +13:59:10.27 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 01:46:31.396 +13:59:10.27
Angular distance between the image centers 0.0383 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits (2nd new image)
verification OK: wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:46:28.874 +13:59:44.33 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 01:46:28.874 +13:59:44.33
Angular distance between the image centers 0.0451 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 01:46:31.396 +13:59:10.27
Second-epoch second image center 01:46:28.874 +13:59:44.33
Angular distance between the image centers 0.01391 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits &> /tmp/tmp.TmtbgwHYxo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.rcWiJvcrf0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_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_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits &> /tmp/tmp.UF1qR5lAhL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits &> /tmp/tmp.2XQli6Wapa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-03-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Found non-empty wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits and wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
The reference image (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits) and catalog (wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat) found
'wcs_Psc-03-Q1b1x1_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 22.950100
a=0.000000 b=1.000000 c=22.950100
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7679 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 18.3962 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (aperture=6.0)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Forced-photometry filter: calibrated wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -> calib.txt_param_ref_wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
2.0 pix Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
2.1 pix fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
2.1 pix fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
Limiting magnitude estimates:
15.4 mag. Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
15.2 mag. Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
15.3 mag. fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
15.3 mag. fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.2 (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.TmtbgwHYxo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'wcs_Psc-03-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=0, passed=7679
Got 7679 stars (including 7121 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.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 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
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 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 7679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 4873 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits N_match=4873 sigma_overall_arcsec=0.237 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.223 sigma_q3_arcsec=0.217 sigma_q4_arcsec=0.200 n_q1=1261 n_q2=1216 n_q3=1199 n_q4=1197 worst_quadrant_to_overall_ratio=1.365
The image catalog is written to wcs_Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits -region wcs_Psc-03-Q1b1x1_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-Q1b1x1_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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.rcWiJvcrf0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Psc-03-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=519, bad_region=0, passed=6762
Got 6762 stars (including 6236 good ones) from the SExtractor catalog wcs_Psc-03-Q1b1x1_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 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 6762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-03-Q1b1x1_2026-01-20_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits N_match=4878 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.239 n_q1=1250 n_q2=1227 n_q3=1200 n_q4=1201 worst_quadrant_to_overall_ratio=1.449
The image catalog is written to wcs_Psc-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Psc-03-Q1b1x1_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-Q1b1x1_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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.UF1qR5lAhL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=458, bad_region=0, passed=7208
Got 7208 stars (including 6737 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat
util/solve_plate_with_UCAC5 got 7208 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 7208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4872 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(), 7208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 7208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4869 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4869 robust_rms=10.689 arcsec worst_quadrant_rms=11.884 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.400 arcsec worst_quadrant_rms=0.431 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.273 arcsec worst_quadrant_rms=0.301 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=1.004 arcsec robust_rms_before_corrected=0.274 arcsec robust_rms_after=0.273 arcsec worst_quadrant_rms_before=0.314 worst_quadrant_rms_after=0.301
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.314 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits N_match=4869 sigma_overall_arcsec=0.280 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.257 sigma_q4_arcsec=0.249 n_q1=1321 n_q2=1188 n_q3=1196 n_q4=1164 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits -region wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2XQli6Wapa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
WCS_IMAGE_NAME=wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
WCS-calibrated image found: wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
Checking if the catalog wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
WCS catalog name: wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=480, bad_region=0, passed=7208
Got 7208 stars (including 6719 good ones) from the SExtractor catalog wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat
util/solve_plate_with_UCAC5 got 7208 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 7208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4872 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4872 robust_rms=10.851 arcsec worst_quadrant_rms=11.750 arcsec
SIP_REFIT: SIP order 3 trial: matched=4872 robust_rms=0.460 arcsec worst_quadrant_rms=0.488 arcsec
SIP_REFIT: SIP order 5 trial: matched=4872 robust_rms=0.313 arcsec worst_quadrant_rms=0.361 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4872 robust_rms_before=1.033 arcsec robust_rms_before_corrected=0.315 arcsec robust_rms_after=0.313 arcsec worst_quadrant_rms_before=0.364 worst_quadrant_rms_after=0.361
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.364 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits N_match=4872 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.334 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.281 n_q1=1317 n_q2=1192 n_q3=1199 n_q4=1164 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits -region wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits'
Saving the final (post-refit) wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits'
Saving the final (post-refit) wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits to local_wcs_cache/
'wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits' -> 'local_wcs_cache/wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits sigma_overall=0.237 worst_q_ratio=1.365
ref2=Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits sigma_overall=0.294 worst_q_ratio=1.449
new1=fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits sigma_overall=0.280 worst_q_ratio=1.130
new2=fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits sigma_overall=0.325 worst_q_ratio=1.155
reference average sigma_overall=0.2655 worst_q_ratio=1.407
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188_astrometric_residuals.png (4873 matched stars from wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.21 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139_astrometric_residuals.png (4878 matched stars from wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352_astrometric_residuals.png (4869 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353_astrometric_residuals.png (4872 matched stars from wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-43-08_20.00sec_0.00C_LIGHTs_0352.fits'
Saving fully-calibrated image wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Psc-03-Q1b1x1_054512_TTUQ1b1x1_3649606_yon7cDVj/wcs_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353.fits'
Preparing the HTML report for the field Psc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:13.56 +10:16:02.7: 11.44 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:15:55.14 +12:40:42.5: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 01:44:57.58 +10:22:19.0: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits at 02:14:03.93 +12:47:10.6: 12.50 +/- 0.02 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:13.56 +10:16:02.7: 11.46 +/- 0.01 detection
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 01:44:57.58 +10:22:19.0: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:15:55.14 +12:40:42.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-03-Q1b1x1_2026-01-20_21-41-00_20.00sec_-15.00C_LIGHT_0139.fits at 02:14:03.93 +12:47:10.6: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 02:15:13.56 +10:16:02.7: ref_mag=11.45 +/- 0.01 new_mean_mag=11.7456 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:14:03.93 +12:47:10.6: ref_mag=12.47 +/- 0.01 new_mean_mag=12.3964 delta=0.08 (need > 0.90)
Adding exclusion_list_local.txt__out20188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20251.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20094_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 20094_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 20095_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 20095_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:28:36.35 +14:39:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20188_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 20188_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 20251_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 20251_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 20260_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 20260_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51697_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51697_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51699_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51699_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51700_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51700_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51703_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51703_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51708_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51708_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 51710_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51710_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51712_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51712_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51716_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51716_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51718_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51718_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51719_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51719_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51722_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51722_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51723_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51723_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51725_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51725_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:26:20.58 +17:42:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51727_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51727_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:45:28.85 +17:08:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51728_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51728_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51732_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51732_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 51834_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51834_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 02:15:55.13 +12:40:42.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51900_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 51900_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:44:57.58 +10:22:19.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51984_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 51984_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52166_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52166_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52179_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52179_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:47:13.23 +17:54:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52184_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52184_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:39:44.53 +16:26:01.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52210_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52210_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:43:49.97 +14:26:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52213_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52213_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52218_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52218_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52245_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52245_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52256_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52256_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52333_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52333_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52374_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52374_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52420_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52420_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 02:02:42.98 +13:27:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52466_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52466_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52496_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52496_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52601_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52601_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52626_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52626_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52666_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52666_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52678_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52678_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52694_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52694_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52706_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52706_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52710_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52710_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52731_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52731_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52749_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52749_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52752_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52752_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52757_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52757_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52760_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52760_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52790_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52790_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52792_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52792_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52794_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52794_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52807_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52807_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52809_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52809_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52810_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52810_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52815_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52815_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52818_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
Preparing report for the candidate 52818_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
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Considering the candidate 52823_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52823_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52829_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52829_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52830_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52830_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52833_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52833_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52842_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52842_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52856_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52856_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52858_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52858_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52859_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52859_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52860_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52860_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52865_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52865_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52867_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52867_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52869_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52869_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52870_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52870_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52876_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52876_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52877_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52877_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52878_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52878_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52879_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52879_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52884_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52884_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52887_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52887_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52891_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52891_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52894_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52894_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52900_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52900_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52907_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52907_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52910_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52910_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52911_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52911_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52912_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52912_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52915_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52915_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52920_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52920_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52922_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52922_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52923_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52923_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52924_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52924_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52928_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52928_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52941_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52941_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52946_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52946_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52952_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52952_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52965_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52965_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52968_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52968_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52969_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52969_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52974_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52974_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52976_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52976_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52977_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52977_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52978_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52978_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52985_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52985_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52992_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52992_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 52995_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 52995_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53002_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53002_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53004_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53004_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53011_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53011_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53012_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53012_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53013_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53013_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53018_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53018_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53020_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53020_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 53056_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 53056_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 29370_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353
The candidate 29370_fd_Psc-03-Q1b1x1_2026-09-09_05-44-25_20.00sec_0.00C_LIGHTs_0353 did not pass the final checks
