This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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 10 09.4170* 09 33 05.40 +15 11 09.1 7.2 U Leo 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,2461322.9170,7.18,0.05,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 20261009.4170 7.18CV 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
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 10 09.4170* 09 32 55.19 +15 12 07.4 7.3 U Leo 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,2461322.9170,7.26,0.05,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 20261009.4170 7.26CV 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
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 10 09.4170* 09 32 37.56 +15 13 41.8 7.7 U Leo 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,2461322.9170,7.71,0.05,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 20261009.4170 7.71CV 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 10 09.4170 2461322.9170 10.61 09:21:00.95 +10:55:40.7
220.46657 38.10693 galactic Cnc Second-epoch detections are separated by 0.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.6 Hebe 0 1 1 10.8 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:21:00.95 +10:55:40.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:21:00.95 +10:55:40.7: 15.72 +/- 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,2461322.9170,10.61,0.05,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 20261009.4170 10.61CV 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
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 10 09.4170* 09 32 55.18 +15 12 07.7 7.6 U Leo 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,2461322.9170,7.57,0.05,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 20261009.4170 7.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 10 09.4170* 09 33 05.43 +15 11 09.0 7.6 U Leo 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,2461322.9170,7.57,0.05,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 20261009.4170 7.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 10 09.4170* 09 32 37.54 +15 13 42.1 7.8 U Leo 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,2461322.9170,7.80,0.05,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 20261009.4170 7.80CV 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 10 09.4170 2461322.9170 12.02 09:38:11.00 +13:44:13.6
219.47735 43.09730 galactic Leo Second-epoch detections are separated by 1.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.52 Europa -0 0 0 12.3 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:38:11.00 +13:44:13.6: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:38:11.00 +13:44:13.6: 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 10 09.4170* 09 38 11.00 +13 44 13.6 12.0 U Leo 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,2461322.9170,12.02,0.05,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 20261009.4170 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4170 2461322.9170 11.62 10:05:38.94 +09:49:01.9
228.77036 47.31428 galactic Leo Second-epoch detections are separated by 0.2" 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.10 Hygiea -0 -0 1 11.8 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:05:38.94 +09:49:01.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:05:38.94 +09:49:01.9: 15.87 +/- 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 10 09.4170* 10 05 38.94 +09 49 01.9 11.6 U Leo 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,2461322.9170,11.62,0.05,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 20261009.4170 11.62CV 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 10 09.4170 2461322.9170 12.46 09:57:53.48 +18:04:07.3
216.34971 49.14048 galactic Leo Second-epoch detections are separated by 1.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.196 Philomela 0 -0 0 12.9 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:57:53.48 +18:04:07.3: 15.13 +/- 0.17 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:57:53.48 +18:04:07.3: 14.78 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.10
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 10 09.4170* 09 57 53.48 +18 04 07.3 12.5 U Leo 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,2461322.9170,12.46,0.05,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 20261009.4170 12.46CV 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 10 09.4170 2461322.9170 12.12 10:12:44.83 +10:30:13.3
229.17255 49.17184 galactic Leo Second-epoch detections are separated by 0.3" 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.16 Psyche -0 -0 1 12.2 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:44.83 +10:30:13.3: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:44.83 +10:30:13.3: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 09.4170* 10 12 44.83 +10 30 13.3 12.1 U Leo 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,2461322.9170,12.12,0.05,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 20261009.4170 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4170 2461322.9170 12.81 09:42:36.83 +12:37:01.4
221.50046 43.60064 galactic Leo Second-epoch detections are separated by 0.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.747 Winchester -0 0 0 13.3 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:42:36.83 +12:37:01.4: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:42:36.83 +12:37:01.4: 16.13 +/- 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 10 09.4170* 09 42 36.83 +12 37 01.4 12.8 U Leo 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,2461322.9170,12.81,0.05,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 20261009.4170 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4170 2461322.9170 13.66 09:30:44.75 +11:21:55.5
221.31328 40.44312 galactic Leo Second-epoch detections are separated by 1.2" 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.584 Semiramis 0 0 0 13.8 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:44.75 +11:21:55.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:44.75 +11:21:55.5: 15.97 +/- 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 10 09.4170* 09 30 44.75 +11 21 55.5 13.7 U Leo 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,2461322.9170,13.66,0.05,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 20261009.4170 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4170 2461322.9170 13.88 09:45:26.66 +16:00:28.6
217.54711 45.61338 galactic Leo Second-epoch detections are separated by 1.4" 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.104 Klymene 0 -1 1 14.2 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:45:26.66 +16:00:28.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:45:26.66 +16:00:28.6: 16.18 +/- 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 10 09.4170* 09 45 26.66 +16 00 28.6 13.9 U Leo 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,2461322.9170,13.88,0.05,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 20261009.4170 13.88CV 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 10 09.4170 2461322.9170 13.87 09:54:57.38 +14:56:27.9
220.28606 47.29600 galactic Leo Second-epoch detections are separated by 0.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.487 Venetia 0 0 0 13.9 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:54:57.38 +14:56:27.9: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:54:57.38 +14:56:27.9: 16.18 +/- 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 10 09.4170* 09 54 57.38 +14 56 27.9 13.9 U Leo 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,2461322.9170,13.87,0.05,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 20261009.4170 13.87CV 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 10 09.4170 2461322.9170 14.07 09:58:26.33 +16:08:19.9
219.14484 48.54235 galactic Leo Second-epoch detections are separated by 0.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.351 Yrsa 1 -0 1 14.2 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:58:26.33 +16:08:19.9: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:58:26.33 +16:08:19.9: 16.04 +/- 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 10 09.4170* 09 58 26.33 +16 08 19.9 14.1 U Leo 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,2461322.9170,14.07,0.05,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 20261009.4170 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4170 2461322.9170 13.40 09:43:56.88 +17:56:25.5
214.78163 45.99592 galactic Leo Second-epoch detections are separated by 0.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.245 Vera -2 -2 3 13.9 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:43:56.88 +17:56:25.5: 15.54 +/- 0.24 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:43:56.88 +17:56:25.5: 15.51 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.53 +/- 0.17
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 10 09.4170* 09 43 56.88 +17 56 25.5 13.4 U Leo 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,2461322.9170,13.40,0.05,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 20261009.4170 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
First image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461322.91737811 09.10.2026 10:00:51.469 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.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.: -7.39
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6963
Objects passed selection criteria: 6953
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 5881.75
Average stars matched: 5785 (98.3551 %)
Memory usage VmPeak: 240448 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 05:11:37 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: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
First image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461322.91737811 09.10.2026 10:00:51.469 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 28
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.11
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 37984
Objects passed selection criteria: 37907
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 32277.5
Average stars matched: 30883.8 (95.682 %)
Memory usage VmPeak: 261628 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 05:13:02 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/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461322.91664429
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:46:31.656 +14:00:33.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Image size: 945.3'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:35.685 +14:01:22.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:31.656 +14:00:33.25
Second-epoch image center 09:46:35.685 +14:01:22.05
Angular distance between the image centers 0.0212 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Image size: 945.1'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:33.207 +14:00:50.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:31.656 +14:00:33.25
Second-epoch image center 09:46:33.207 +14:00:50.83
Angular distance between the image centers 0.0079 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 09:46:35.685 +14:01:22.05
Second-epoch second image center 09:46:33.207 +14:00:50.83
Angular distance between the image centers 0.01325 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/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.qkel5oHihx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.Urs962Yz6d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits &> /tmp/tmp.9gTAADvruZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits &> /tmp/tmp.yh9zZdZIsN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat' -> 'wcsmag.cat'
Read 7795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4767 to 154.9673 deg, Dec +8.5555 to +19.3045 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 138.4767 to 154.9673 deg, Dec 8.5555 to 19.3045 deg
Loaded 4795 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): 3891 out of 4080 total matches.
Matched with Tycho-2 4080 out of 7795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.915200
a=0.000000 b=1.000000 c=22.915200
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4767 to 154.9673 deg, Dec +8.5555 to +19.3045 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 138.4767 to 154.9673 deg, Dec 8.5555 to 19.3045 deg
Loaded 4795 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): 3891 out of 4080 total matches.
Matched with Tycho-2 4080 out of 7795 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (aperture=6.6)
Read 7228 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4289 to 155.2668 deg, Dec +8.1760 to +19.5844 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 138.4289 to 155.2668 deg, Dec 8.1760 to 19.5844 deg
Loaded 5216 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): 3897 out of 4082 total matches.
Matched with Tycho-2 4082 out of 7228 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (aperture=6.2)
____ 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:
2.4 pix Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.1 pix Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Limiting magnitude estimates:
15.5 mag. Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.5 mag. Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
14.4 mag. fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
14.4 mag. fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.qkel5oHihx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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=485, bad_region=0, passed=7795
Got 7795 stars (including 7304 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
util/solve_plate_with_UCAC5 got 7795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4624 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 4604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 7795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4624 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 7795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 7795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4604 stars left (next iteration limit 5064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=4604 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.439 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.381 n_q1=1374 n_q2=1044 n_q3=1180 n_q4=1006 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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.Urs962Yz6d (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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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=490, bad_region=0, passed=7228
Got 7228 stars (including 6724 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7228 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 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4626 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 4607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 7228 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 19.6)
Done reading UCAC5 zone files...
Matched 4626 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 7228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 7228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4607 stars left (next iteration limit 5067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=4607 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.285 n_q1=1021 n_q2=1212 n_q3=1021 n_q4=1353 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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.9gTAADvruZ (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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.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=217, bad_region=0, passed=4309
Got 4309 stars (including 4087 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat
util/solve_plate_with_UCAC5 got 4309 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.3'
Seting catalog search parameters based on the expected field of view 945.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013129 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010503 (37.8 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 3796 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3780 matched stars entering correct_measured_positions(), 3781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3780 matched stars entering correct_measured_positions(), 4309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 3795 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3780 matched stars entering correct_measured_positions(), 4309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 3780 matched stars entering correct_measured_positions(), 4309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3780 stars left (next iteration limit 4158)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3780 robust_rms=10.022 arcsec worst_region_rms=19.173 arcsec outer_annulus_rms=19.173 arcsec
SIP_REFIT: SIP order 3 trial: matched=3780 robust_rms=0.592 arcsec worst_region_rms=0.938 arcsec outer_annulus_rms=0.748 arcsec
SIP_REFIT: SIP order 5 trial: matched=3780 robust_rms=0.367 arcsec worst_region_rms=0.481 arcsec outer_annulus_rms=0.418 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3780 robust_rms_before=1.663 arcsec robust_rms_before_corrected=0.399 arcsec robust_rms_after=0.367 arcsec worst_region_rms_before=0.479 worst_region_rms_after=0.481 outer_annulus_rms_before=1.807 outer_annulus_rms_after=0.418
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.479 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits worst_region_rms_kept=0.479 arcsec robust_rms_kept=0.399 arcsec matched=3780
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits N_match=3780 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.497 sigma_q3_arcsec=0.355 sigma_q4_arcsec=0.414 n_q1=1219 n_q2=676 n_q3=1110 n_q4=775 worst_quadrant_to_overall_ratio=1.238
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.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.yh9zZdZIsN (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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.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=218, bad_region=0, passed=4329
Got 4329 stars (including 4107 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 4329 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 3806 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3789 matched stars entering correct_measured_positions(), 3789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3789 matched stars entering correct_measured_positions(), 4329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 3807 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3790 matched stars entering correct_measured_positions(), 4329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 3790 matched stars entering correct_measured_positions(), 4329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3790 stars left (next iteration limit 4167)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3790 robust_rms=10.343 arcsec worst_region_rms=19.621 arcsec outer_annulus_rms=19.621 arcsec
SIP_REFIT: SIP order 3 trial: matched=3790 robust_rms=0.558 arcsec worst_region_rms=0.838 arcsec outer_annulus_rms=0.763 arcsec
SIP_REFIT: SIP order 5 trial: matched=3790 robust_rms=0.373 arcsec worst_region_rms=0.513 arcsec outer_annulus_rms=0.439 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3790 robust_rms_before=1.612 arcsec robust_rms_before_corrected=0.399 arcsec robust_rms_after=0.373 arcsec worst_region_rms_before=0.486 worst_region_rms_after=0.513 outer_annulus_rms_before=1.840 outer_annulus_rms_after=0.439
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.486 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits worst_region_rms_kept=0.486 arcsec robust_rms_kept=0.399 arcsec matched=3790
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits N_match=3790 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.375 sigma_q2_arcsec=0.511 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.403 n_q1=1219 n_q2=689 n_q3=1097 n_q4=785 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.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_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
Saving the final (post-refit) wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
Saving the final (post-refit) wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits'
Saving the final (post-refit) wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits sigma_overall=0.389 worst_q_ratio=1.128
ref2=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits sigma_overall=0.309 worst_q_ratio=1.071
new1=fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits sigma_overall=0.401 worst_q_ratio=1.238
new2=fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits sigma_overall=0.388 worst_q_ratio=1.316
reference average sigma_overall=0.349 worst_q_ratio=1.0995
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155_astrometric_residuals.png (4604 matched stars from wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138_astrometric_residuals.png (4607 matched stars from wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502_astrometric_residuals.png (3780 matched stars from wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503_astrometric_residuals.png (3790 matched stars from wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits'
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:21:00.95 +10:55:40.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:21:00.95 +10:55:40.7: 15.72 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20371.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 28s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20363_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 20363_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20364_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 20364_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20365_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 20365_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20366_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 20366_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
**** FOUND 09:35:55.56 +14:22:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20371_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 20371_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 32s
Prepared the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:21:00.95 +10:55:40.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:46:31.656 +14:00:33.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Image size: 945.3'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:35.685 +14:01:22.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:31.656 +14:00:33.25
Second-epoch image center 09:46:35.685 +14:01:22.05
Angular distance between the image centers 0.0212 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Image size: 945.1'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:33.207 +14:00:50.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:31.656 +14:00:33.25
Second-epoch image center 09:46:33.207 +14:00:50.83
Angular distance between the image centers 0.0079 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 09:46:35.685 +14:01:22.05
Second-epoch second image center 09:46:33.207 +14:00:50.83
Angular distance between the image centers 0.01325 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/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.DMPrIMboGk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.3cqW5ohyLe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits &> /tmp/tmp.fGdoSHr3f5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits &> /tmp/tmp.jzVaI43REc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat' -> 'wcsmag.cat'
Read 41224 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4693 to 154.9673 deg, Dec +8.5466 to +19.3048 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 138.4693 to 154.9673 deg, Dec 8.5466 to 19.3048 deg
Loaded 4807 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): 3691 out of 4110 total matches.
Matched with Tycho-2 4110 out of 41224 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.790900
a=0.000000 b=1.000000 c=22.790900
From vast_summary.log: estimated ref. image limiting mag.: -7.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 41224 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4693 to 154.9673 deg, Dec +8.5466 to +19.3048 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 138.4693 to 154.9673 deg, Dec 8.5466 to 19.3048 deg
Loaded 4807 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): 3691 out of 4110 total matches.
Matched with Tycho-2 4110 out of 41224 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (aperture=5.1)
Read 42226 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3847 to 155.2957 deg, Dec +8.1204 to +19.5912 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 138.3847 to 155.2957 deg, Dec 8.1204 to 19.5912 deg
Loaded 5273 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): 3733 out of 4126 total matches.
Matched with Tycho-2 4126 out of 42226 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.0 pix Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.5 pix fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
2.5 pix fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Limiting magnitude estimates:
15.7 mag. Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.7 mag. Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
14.6 mag. fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
14.7 mag. fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DMPrIMboGk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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=22, blended=1984, bad_region=0, passed=41202
Got 41202 stars (including 39163 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
util/solve_plate_with_UCAC5 got 41202 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4609 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 4594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 41202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4609 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 41202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 41202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4593 stars left (next iteration limit 5052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=4593 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.435 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.373 n_q1=1357 n_q2=1062 n_q3=1139 n_q4=1035 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.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.3cqW5ohyLe (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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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=16, blended=1796, bad_region=34, passed=42210
Got 42210 stars (including 40321 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 42210 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 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 4604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 42210 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 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 42210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 42210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4604 stars left (next iteration limit 5064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=4604 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.314 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.270 n_q1=1022 n_q2=1221 n_q3=1021 n_q4=1340 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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.fGdoSHr3f5 (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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=661, bad_region=43, passed=23262
Got 23262 stars (including 22525 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat
util/solve_plate_with_UCAC5 got 23262 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.3'
Seting catalog search parameters based on the expected field of view 945.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013129 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010503 (37.8 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 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4632 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4615 matched stars entering correct_measured_positions(), 4616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4615 matched stars entering correct_measured_positions(), 23262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4632 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 23262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4616 matched stars entering correct_measured_positions(), 23262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4616 stars left (next iteration limit 5076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4616 robust_rms=9.674 arcsec worst_region_rms=19.124 arcsec outer_annulus_rms=19.124 arcsec
SIP_REFIT: SIP order 3 trial: matched=4616 robust_rms=0.584 arcsec worst_region_rms=0.915 arcsec outer_annulus_rms=0.770 arcsec
SIP_REFIT: SIP order 5 trial: matched=4616 robust_rms=0.378 arcsec worst_region_rms=0.490 arcsec outer_annulus_rms=0.431 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4616 robust_rms_before=1.666 arcsec robust_rms_before_corrected=0.382 arcsec robust_rms_after=0.378 arcsec worst_region_rms_before=0.476 worst_region_rms_after=0.490 outer_annulus_rms_before=1.841 outer_annulus_rms_after=0.431
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.476 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits worst_region_rms_kept=0.476 arcsec robust_rms_kept=0.382 arcsec matched=4616
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits N_match=4616 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.501 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.411 n_q1=1459 n_q2=781 n_q3=1431 n_q4=945 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.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.jzVaI43REc (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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.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_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.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=2, blended=677, bad_region=44, passed=23454
Got 23454 stars (including 22696 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 23454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4635 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4618 matched stars entering correct_measured_positions(), 4618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4618 matched stars entering correct_measured_positions(), 23454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4635 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4620 matched stars entering correct_measured_positions(), 23454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4620 matched stars entering correct_measured_positions(), 23454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4620 stars left (next iteration limit 5079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4620 robust_rms=9.916 arcsec worst_region_rms=19.471 arcsec outer_annulus_rms=19.471 arcsec
SIP_REFIT: SIP order 3 trial: matched=4620 robust_rms=0.557 arcsec worst_region_rms=0.765 arcsec outer_annulus_rms=0.742 arcsec
SIP_REFIT: SIP order 5 trial: matched=4620 robust_rms=0.384 arcsec worst_region_rms=0.506 arcsec outer_annulus_rms=0.444 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4620 robust_rms_before=1.606 arcsec robust_rms_before_corrected=0.381 arcsec robust_rms_after=0.384 arcsec worst_region_rms_before=0.465 worst_region_rms_after=0.506 outer_annulus_rms_before=1.804 outer_annulus_rms_after=0.444
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.465 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits worst_region_rms_kept=0.465 arcsec robust_rms_kept=0.381 arcsec matched=4620
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits N_match=4620 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.362 sigma_q2_arcsec=0.469 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.400 n_q1=1451 n_q2=796 n_q3=1425 n_q4=948 worst_quadrant_to_overall_ratio=1.240
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/wcs_fd_Leo-04-Q1b1x1_2026-10-09_04-59-48_20.00sec_-0.00C_LIGHTs_0502.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q1b1x1_050541_TTUQ1b1x1_119501_TWWUjtRC/wcs_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503.fits
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:16:29.65 +09:14:59.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:16:40.77 +08:45:56.2: 10.43 +/- 0.00 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:16:36.18 +08:37:40.6: 11.32 +/- 0.01 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:38:11.00 +13:44:13.6: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:35:22.22 +12:12:45.5: 14.44 +/- 0.08 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:05:38.94 +09:49:01.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:16:36.18 +08:37:40.6: 11.07 +/- 0.01 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:16:29.65 +09:14:59.4: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:35:22.22 +12:12:45.5: 14.43 +/- 0.08 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:38:11.00 +13:44:13.6: 16.14 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 10:16:36.18 +08:37:40.6: ref_mag=11.17 +/- 0.00 new_mean_mag=11.2629 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry reference-image weighted average: 14.44 +/- 0.06
Forced photometry filter REJECTED candidate at 10:16:29.65 +09:14:59.4: ref_mag=12.55 +/- 0.01 new_mean_mag=12.5026 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:35:22.22 +12:12:45.5: ref_mag=14.44 +/- 0.06 new_mean_mag=14.4101 delta=0.03 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:16:40.77 +08:45:56.2: 10.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.26 +/- 0.00
Forced photometry filter REJECTED candidate at 10:16:40.77 +08:45:56.2: ref_mag=10.26 +/- 0.00 new_mean_mag=10.3191 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:05:38.94 +09:49:01.9: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:57:53.48 +18:04:07.3: 15.13 +/- 0.17 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:44.83 +10:30:13.3: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:42:36.83 +12:37:01.4: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:17:25.77 +16:32:42.2: 13.15 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:57:53.48 +18:04:07.3: 14.78 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.10
Forced photometry filter KEPT candidate at 09:57:53.48 +18:04:07.3: ref_mag=14.91 +/- 0.10 new_mean_mag=12.4641 delta=2.44 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:44.83 +10:30:13.3: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:42:36.83 +12:37:01.4: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:17:25.77 +16:32:42.2: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter REJECTED candidate at 09:17:25.77 +16:32:42.2: ref_mag=13.27 +/- 0.03 new_mean_mag=13.4978 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:44.75 +11:21:55.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:44.75 +11:21:55.5: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:45:26.66 +16:00:28.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:45:26.66 +16:00:28.6: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:54:57.38 +14:56:27.9: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:58:26.33 +16:08:19.9: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:43:56.88 +17:56:25.5: 15.54 +/- 0.24 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:54:57.38 +14:56:27.9: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:58:26.33 +16:08:19.9: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:43:56.88 +17:56:25.5: 15.51 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.53 +/- 0.17
Forced photometry filter KEPT candidate at 09:43:56.88 +17:56:25.5: ref_mag=15.53 +/- 0.17 new_mean_mag=13.4034 delta=2.12 (need > 0.90)
Adding exclusion_list_local.txt__out31418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55120.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 76s
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: 10s
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Considering the candidate 54786_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54786_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
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Considering the candidate 54794_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54794_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
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Considering the candidate 54800_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54800_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 54802_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54802_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54803_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54803_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54804_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54804_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54811_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54811_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
**** FOUND 09:21:00.94 +10:55:40.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54817_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54817_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
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Considering the candidate 54840_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54840_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
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Considering the candidate 54841_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54841_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54845_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54845_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
**** FOUND 09:40:58.92 +09:52:39.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 54849_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54849_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54867_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54867_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
**** FOUND 10:08:08.91 +11:58:15.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 54876_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54876_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54903_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54903_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
**** FOUND 09:51:35.85 +17:28:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54910_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54910_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54922_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 54922_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 54939_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 54939_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
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Considering the candidate 55034_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 55034_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
**** FOUND 09:19:41.68 +10:49:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55037_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 55037_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 55074_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 55074_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 55092_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 55092_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 55120_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 55120_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 31418_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
Preparing report for the candidate 31418_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
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Considering the candidate 39281_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503
The candidate 39281_fd_Leo-04-Q1b1x1_2026-10-09_05-00-51_20.00sec_0.00C_LIGHTs_0503 did not pass the final checks
