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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe
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 09.4169* 09 33 05.78 +15 11 08.6 7.0 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,2461322.9169,7.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 7.01CV 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 09.4169* 09 32 55.10 +15 12 09.1 7.1 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,2461322.9169,7.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 7.12CV 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
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 09.4169* 09 32 37.52 +15 13 42.9 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,2461322.9169,7.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 7.58CV 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 09.4169 2461322.9169 10.67 09:21:00.93 +10:55:40.4
220.46662 38.10682 galactic Cnc Second-epoch detections are separated by 1.3" and 10.6 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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:21:00.93 +10:55:40.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:21:00.93 +10:55:40.4: 99.00 +/- 99.00 bad_region
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,2461322.9169,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 10.67CV 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 09.4169 2461322.9169 14.17 09:44:03.83 +17:26:33.7
215.46373 45.84319 galactic Leo Second-epoch detections are separated by 1.6" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.535 Montague 0 -1 1 14.9 0 0
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:44:03.83 +17:26:33.7: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:44:03.83 +17:26:33.7: 15.99 +/- 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 09.4169* 09 44 03.83 +17 26 33.7 14.2 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,2461322.9169,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 14.17CV 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 09.4169* 09 32 55.11 +15 12 08.9 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,2461322.9169,7.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 7.58CV 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 09.4169* 09 33 05.80 +15 11 08.7 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,2461322.9169,7.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 7.58CV 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 09.4169* 09 32 37.52 +15 13 43.0 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,2461322.9169,7.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 7.79CV 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 09.4169 2461322.9169 12.00 09:38:10.97 +13:44:13.6
219.47728 43.09719 galactic Leo Second-epoch detections are separated by 0.7" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.52 Europa -0 0 0 12.3 0 0
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:38:10.97 +13:44:13.6: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:38:10.97 +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 09.4169* 09 38 10.97 +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,2461322.9169,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 12.00CV 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 09.4169 2461322.9169 12.50 09:57:53.44 +18:04:07.1
216.34970 49.14031 galactic Leo Second-epoch detections are separated by 0.7" and 9.9 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 -1 1 12.9 0 0
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:57:53.44 +18:04:07.1: 15.19 +/- 0.18 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:57:53.44 +18:04:07.1: 14.83 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.11
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 09.4169* 09 57 53.44 +18 04 07.1 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,2461322.9169,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 12.50CV 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 09.4169 2461322.9169 12.73 09:42:36.82 +12:37:00.8
221.50065 43.60053 galactic Leo Second-epoch detections are separated by 2.2" and 10.5 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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:42:36.82 +12:37:00.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:42:36.82 +12:37:00.8: 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 09.4169* 09 42 36.82 +12 37 00.8 12.7 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,2461322.9169,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4169 2461322.9169 13.56 09:30:44.81 +11:21:55.9
221.31329 40.44339 galactic Leo Second-epoch detections are separated by 1.6" and 10.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.584 Semiramis 1 0 1 13.8 -0 0
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:44.81 +11:21:55.9: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:44.81 +11:21:55.9: 15.96 +/- 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 09.4169* 09 30 44.81 +11 21 55.9 13.6 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,2461322.9169,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 13.56CV 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 09.4169 2461322.9169 13.86 09:45:26.64 +16:00:29.5
217.54674 45.61341 galactic Leo Second-epoch detections are separated by 2.6" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.104 Klymene 0 0 0 14.2 0 0
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:45:26.64 +16:00:29.5: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:45:26.64 +16:00:29.5: 16.19 +/- 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 09.4169* 09 45 26.64 +16 00 29.5 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,2461322.9169,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4169 2461322.9169 13.78 09:54:57.37 +14:56:27.6
220.28615 47.29593 galactic Leo Second-epoch detections are separated by 1.3" and 10.0 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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:54:57.37 +14:56:27.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:54:57.37 +14:56:27.6: 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 09.4169* 09 54 57.37 +14 56 27.6 13.8 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,2461322.9169,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4169 2461322.9169 13.38 09:43:56.86 +17:56:26.3
214.78129 45.99593 galactic Leo Second-epoch detections are separated by 1.8" and 9.8 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 -1 3 13.9 -0 0
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:43:56.86 +17:56:26.3: 15.54 +/- 0.24 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:43:56.86 +17:56:26.3: 15.50 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.52 +/- 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 09.4169* 09 43 56.86 +17 56 26.3 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,2461322.9169,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4169 13.38CV 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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461322.91722716 09.10.2026 10:00:38.427 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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): 4966
Objects passed selection criteria: 4961
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 4529.5
Average stars matched: 4104.25 (90.6115 %)
Memory usage VmPeak: 232592 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 06:13:24 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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461322.91722716 09.10.2026 10:00:38.427 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.10
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: 9 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): 29327
Objects passed selection criteria: 29257
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 26445.2
Average stars matched: 23804.5 (90.0143 %)
Memory usage VmPeak: 256740 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 06:14:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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: 2461322.91651138
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Image size: 941.2'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:46:39.271 +13:57:47.31 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 09:46:39.271 +13:57:47.31
Angular distance between the image centers 0.0554 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Image size: 941.0'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:46:36.793 +13:58:35.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:31.656 +14:00:33.25
Second-epoch image center 09:46:36.793 +13:58:35.60
Angular distance between the image centers 0.0387 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 09:46:39.271 +13:57:47.31
Second-epoch second image center 09:46:36.793 +13:58:35.60
Angular distance between the image centers 0.01674 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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.nGupXWKfP4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.RSeTJbwyRf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits &> /tmp/tmp.TSKQVK6NLy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits &> /tmp/tmp.aPcwThCXOi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.1 pix Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.3 pix fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
2.3 pix fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Limiting magnitude estimates:
15.5 mag. Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.5 mag. Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
14.5 mag. fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
14.5 mag. fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.5 (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.nGupXWKfP4 (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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=485, bad_region=1563, passed=7795
Got 7795 stars (including 5847 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_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 4730 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4715 matched stars entering correct_measured_positions(), 4715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4715 matched stars entering correct_measured_positions(), 6560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4730 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4715 matched stars entering correct_measured_positions(), 6560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4715 matched stars entering correct_measured_positions(), 6560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4715 stars left (next iteration limit 5186)
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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=4715 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.416 sigma_q3_arcsec=0.401 sigma_q4_arcsec=0.365 n_q1=1711 n_q2=767 n_q3=1466 n_q4=771 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q2b1x1_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-Q2b1x1_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.RSeTJbwyRf (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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, bad_region=1848, passed=7228
Got 7228 stars (including 5015 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_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 4551 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4537 matched stars entering correct_measured_positions(), 4537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4537 matched stars entering correct_measured_positions(), 5719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4551 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4537 matched stars entering correct_measured_positions(), 5719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4537 matched stars entering correct_measured_positions(), 5719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4537 stars left (next iteration limit 4990)
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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=4537 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.306 sigma_q4_arcsec=0.310 n_q1=1313 n_q2=791 n_q3=1419 n_q4=1014 worst_quadrant_to_overall_ratio=1.255
The image catalog is written to wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q2b1x1_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-Q2b1x1_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.TSKQVK6NLy (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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=216, bad_region=637, passed=3928
Got 3928 stars (including 3099 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat
util/solve_plate_with_UCAC5 got 3928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 19.2)
Done reading UCAC5 zone files...
Matched 2914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2903 matched stars entering correct_measured_positions(), 2904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2903 matched stars entering correct_measured_positions(), 3414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 19.2)
Done reading UCAC5 zone files...
Matched 2913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2904 matched stars entering correct_measured_positions(), 3414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 2904 matched stars entering correct_measured_positions(), 3414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 2904 stars left (next iteration limit 3193)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2904 robust_rms=6.644 arcsec worst_region_rms=10.323 arcsec outer_annulus_rms=10.323 arcsec
SIP_REFIT: SIP order 3 trial: matched=2904 robust_rms=0.542 arcsec worst_region_rms=0.662 arcsec outer_annulus_rms=0.588 arcsec
SIP_REFIT: SIP order 5 trial: matched=2904 robust_rms=0.399 arcsec worst_region_rms=0.513 arcsec outer_annulus_rms=0.513 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2904 robust_rms_before=1.599 arcsec robust_rms_before_corrected=0.428 arcsec robust_rms_after=0.399 arcsec worst_region_rms_before=0.567 worst_region_rms_after=0.513 outer_annulus_rms_before=1.535 outer_annulus_rms_after=0.513
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.567 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits worst_region_rms_kept=0.567 arcsec robust_rms_kept=0.428 arcsec matched=2904
WCS_QUALITY_DIAG: file=fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits N_match=2904 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.407 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.450 n_q1=1081 n_q2=389 n_q3=986 n_q4=448 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits -region wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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.aPcwThCXOi (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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=235, bad_region=638, passed=3960
Got 3960 stars (including 3109 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat
util/solve_plate_with_UCAC5 got 3960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 2922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2910 matched stars entering correct_measured_positions(), 2911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2910 matched stars entering correct_measured_positions(), 3443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 2922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2910 matched stars entering correct_measured_positions(), 3443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 2910 matched stars entering correct_measured_positions(), 3443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 2910 stars left (next iteration limit 3201)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2910 robust_rms=6.687 arcsec worst_region_rms=10.855 arcsec outer_annulus_rms=10.855 arcsec
SIP_REFIT: SIP order 3 trial: matched=2910 robust_rms=0.537 arcsec worst_region_rms=0.665 arcsec outer_annulus_rms=0.596 arcsec
SIP_REFIT: SIP order 5 trial: matched=2910 robust_rms=0.406 arcsec worst_region_rms=0.519 arcsec outer_annulus_rms=0.519 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2910 robust_rms_before=1.574 arcsec robust_rms_before_corrected=0.436 arcsec robust_rms_after=0.406 arcsec worst_region_rms_before=0.570 worst_region_rms_after=0.519 outer_annulus_rms_before=1.454 outer_annulus_rms_after=0.519
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.570 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits worst_region_rms_kept=0.570 arcsec robust_rms_kept=0.436 arcsec matched=2910
WCS_QUALITY_DIAG: file=fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits N_match=2910 sigma_overall_arcsec=0.428 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.442 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.508 n_q1=1067 n_q2=392 n_q3=987 n_q4=464 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits -region wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
Saving the final (post-refit) wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
Saving the final (post-refit) wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits'
Saving the final (post-refit) wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits sigma_overall=0.376 worst_q_ratio=1.104
ref2=Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits sigma_overall=0.339 worst_q_ratio=1.255
new1=fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits sigma_overall=0.418 worst_q_ratio=1.076
new2=fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits sigma_overall=0.428 worst_q_ratio=1.188
reference average sigma_overall=0.3575 worst_q_ratio=1.1795
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155_astrometric_residuals.png (4715 matched stars from wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138_astrometric_residuals.png (4537 matched stars from wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560_astrometric_residuals.png (2904 matched stars from wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561_astrometric_residuals.png (2910 matched stars from wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits'
Preparing the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:21:00.93 +10:55:40.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:21:00.93 +10:55:40.4: 99.00 +/- 99.00 bad_region
Adding exclusion_list_local.txt__out21639.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21618_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 21618_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21619_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 21619_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21620_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 21620_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21626_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 21626_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
**** FOUND 09:35:55.57 +14:22:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21639_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 21639_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:21:00.93 +10:55:40.4
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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Image size: 941.2'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:46:39.271 +13:57:47.31 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 09:46:39.271 +13:57:47.31
Angular distance between the image centers 0.0554 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Image size: 941.0'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:46:36.793 +13:58:35.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:31.656 +14:00:33.25
Second-epoch image center 09:46:36.793 +13:58:35.60
Angular distance between the image centers 0.0387 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 09:46:39.271 +13:57:47.31
Second-epoch second image center 09:46:36.793 +13:58:35.60
Angular distance between the image centers 0.01674 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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.LPJSo7g5jB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.S0Qu74RxYc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits &> /tmp/tmp.8TvY0Qe2pk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits &> /tmp/tmp.oeMzTJ6sWx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q2b1x1_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.: -7.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.69
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q2b1x1_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 28 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.0 pix Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.2 pix fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
2.2 pix fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Limiting magnitude estimates:
15.7 mag. Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.7 mag. Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
14.6 mag. fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
14.7 mag. fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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.LPJSo7g5jB (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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1984, bad_region=7339, passed=41202
Got 41202 stars (including 32182 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_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 4733 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 4720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 35588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4733 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 35588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 35588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4720 stars left (next iteration limit 5192)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=4720 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.396 sigma_q4_arcsec=0.349 n_q1=1715 n_q2=787 n_q3=1432 n_q4=786 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q2b1x1_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-Q2b1x1_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.S0Qu74RxYc (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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1796, bad_region=9857, passed=42210
Got 42210 stars (including 30951 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_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 4554 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4545 matched stars entering correct_measured_positions(), 4545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4545 matched stars entering correct_measured_positions(), 34434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4554 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4545 matched stars entering correct_measured_positions(), 34434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4545 matched stars entering correct_measured_positions(), 34434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4545 stars left (next iteration limit 4999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=4545 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.326 sigma_q2_arcsec=0.411 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.301 n_q1=1330 n_q2=851 n_q3=1352 n_q4=1012 worst_quadrant_to_overall_ratio=1.275
The image catalog is written to wcs_Leo-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q2b1x1_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-Q2b1x1_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.8TvY0Qe2pk (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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=693, bad_region=2676, passed=22689
Got 22689 stars (including 19403 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat
util/solve_plate_with_UCAC5 got 22689 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4707 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4689 matched stars entering correct_measured_positions(), 4690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4688 matched stars entering correct_measured_positions(), 20715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4705 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4690 matched stars entering correct_measured_positions(), 20715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4690 matched stars entering correct_measured_positions(), 20715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4690 stars left (next iteration limit 5156)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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=4690 robust_rms=6.637 arcsec worst_region_rms=10.240 arcsec outer_annulus_rms=10.240 arcsec
SIP_REFIT: SIP order 3 trial: matched=4690 robust_rms=0.552 arcsec worst_region_rms=0.667 arcsec outer_annulus_rms=0.624 arcsec
SIP_REFIT: SIP order 5 trial: matched=4690 robust_rms=0.416 arcsec worst_region_rms=0.527 arcsec outer_annulus_rms=0.527 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4690 robust_rms_before=1.597 arcsec robust_rms_before_corrected=0.408 arcsec robust_rms_after=0.416 arcsec worst_region_rms_before=0.566 worst_region_rms_after=0.527 outer_annulus_rms_before=1.449 outer_annulus_rms_after=0.527
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.566 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits worst_region_rms_kept=0.566 arcsec robust_rms_kept=0.408 arcsec matched=4690
WCS_QUALITY_DIAG: file=fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits N_match=4690 sigma_overall_arcsec=0.411 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.425 n_q1=1724 n_q2=612 n_q3=1612 n_q4=742 worst_quadrant_to_overall_ratio=1.035
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits -region wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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.oeMzTJ6sWx (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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=813, bad_region=2674, passed=22989
Got 22989 stars (including 19577 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat
util/solve_plate_with_UCAC5 got 22989 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4713 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4695 matched stars entering correct_measured_positions(), 4696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4695 matched stars entering correct_measured_positions(), 21003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4711 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4694 matched stars entering correct_measured_positions(), 21003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4694 matched stars entering correct_measured_positions(), 21003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4694 stars left (next iteration limit 5164)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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=4694 robust_rms=6.649 arcsec worst_region_rms=10.150 arcsec outer_annulus_rms=10.150 arcsec
SIP_REFIT: SIP order 3 trial: matched=4694 robust_rms=0.545 arcsec worst_region_rms=0.640 arcsec outer_annulus_rms=0.620 arcsec
SIP_REFIT: SIP order 5 trial: matched=4694 robust_rms=0.421 arcsec worst_region_rms=0.515 arcsec outer_annulus_rms=0.515 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4694 robust_rms_before=1.583 arcsec robust_rms_before_corrected=0.421 arcsec robust_rms_after=0.421 arcsec worst_region_rms_before=0.537 worst_region_rms_after=0.515 outer_annulus_rms_before=1.409 outer_annulus_rms_after=0.515
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.537 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits worst_region_rms_kept=0.537 arcsec robust_rms_kept=0.421 arcsec matched=4694
WCS_QUALITY_DIAG: file=fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits N_match=4694 sigma_overall_arcsec=0.423 sigma_q1_arcsec=0.430 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.401 sigma_q4_arcsec=0.484 n_q1=1716 n_q2=613 n_q3=1622 n_q4=743 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-04-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits -region wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/wcs_fd_Leo-04-Q2b1x1_2026-10-09_04-59-36_20.00sec_-0.00C_LIGHT_0560.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.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-Q2b1x1_061001_TTUQ2b1x1_3701476_s0G5Vkoe/wcs_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561.fits
Preparing the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:22:22.78 +17:50:35.1: 13.39 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:44:03.83 +17:26:33.7: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:38:10.97 +13:44:13.6: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:24:07.07 +17:17:07.0: 14.26 +/- 0.08 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:21:50.55 +14:00:08.1: 13.03 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:57:53.44 +18:04:07.1: 15.19 +/- 0.18 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:24:07.07 +17:17:07.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:21:50.55 +14:00:08.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:38:10.97 +13:44:13.6: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:44:03.83 +17:26:33.7: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:22:22.78 +17:50:35.1: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 14.26 +/- 0.08
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Forced photometry filter REJECTED candidate at 09:21:50.55 +14:00:08.1: ref_mag=13.03 +/- 0.03 new_mean_mag=13.1938 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:24:07.07 +17:17:07.0: ref_mag=14.26 +/- 0.08 new_mean_mag=14.1800 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter REJECTED candidate at 09:22:22.78 +17:50:35.1: ref_mag=13.39 +/- 0.04 new_mean_mag=13.8416 delta=-0.45 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:42:36.82 +12:37:00.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:57:53.44 +18:04:07.1: 14.83 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.11
Forced photometry filter KEPT candidate at 09:57:53.44 +18:04:07.1: ref_mag=14.96 +/- 0.11 new_mean_mag=12.4955 delta=2.47 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:42:36.82 +12:37:00.8: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:19:23.82 +16:28:03.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:19:41.55 +10:49:42.4: 13.65 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:22:27.32 +13:16:45.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:19:23.82 +16:28:03.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:19:41.55 +10:49:42.4: 99.00 +/- 99.00 bad_region
Forced photometry filter REJECTED candidate at 09:19:23.82 +16:28:03.5: ref_mag=13.30 +/- 0.03 new_mean_mag=13.5069 delta=-0.21 (need > 0.90)
Forced photometry reference-image weighted average: 13.65 +/- 0.05
Forced photometry filter REJECTED candidate at 09:19:41.55 +10:49:42.4: ref_mag=13.65 +/- 0.05 new_mean_mag=13.4717 delta=0.18 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:22:27.32 +13:16:45.9: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry filter REJECTED candidate at 09:22:27.32 +13:16:45.9: ref_mag=13.57 +/- 0.04 new_mean_mag=13.5058 delta=0.07 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:20:18.32 +13:32:41.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:59.44 +10:46:36.8: 13.41 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:44.81 +11:21:55.9: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:20:18.32 +13:32:41.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Forced photometry filter REJECTED candidate at 09:20:18.32 +13:32:41.6: ref_mag=13.68 +/- 0.05 new_mean_mag=13.5975 delta=0.08 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:59.44 +10:46:36.8: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter REJECTED candidate at 09:29:59.44 +10:46:36.8: ref_mag=13.46 +/- 0.03 new_mean_mag=13.4919 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:44.81 +11:21:55.9: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:22:35.60 +17:34:58.1: 14.18 +/- 0.08 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:45:26.64 +16:00:29.5: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:19:54.15 +12:34:45.2: 14.14 +/- 0.08 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:54:57.37 +14:56:27.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:45:26.64 +16:00:29.5: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:22:35.60 +17:34:58.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:19:54.15 +12:34:45.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 14.18 +/- 0.08
Forced photometry filter REJECTED candidate at 09:22:35.60 +17:34:58.1: ref_mag=14.18 +/- 0.08 new_mean_mag=13.9917 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 14.14 +/- 0.08
Forced photometry filter REJECTED candidate at 09:19:54.15 +12:34:45.2: ref_mag=14.14 +/- 0.08 new_mean_mag=13.9720 delta=0.17 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:24:29.31 +17:32:56.2: 14.48 +/- 0.10 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:54:57.37 +14:56:27.6: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:24:29.31 +17:32:56.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 14.48 +/- 0.10
Forced photometry filter REJECTED candidate at 09:24:29.31 +17:32:56.2: ref_mag=14.48 +/- 0.10 new_mean_mag=14.2975 delta=0.18 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:25:26.84 +15:07:34.7: 14.82 +/- 0.13 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:43:56.86 +17:56:26.3: 15.54 +/- 0.24 detection
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:25:26.84 +15:07:34.7: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 14.82 +/- 0.13
Forced photometry filter REJECTED candidate at 09:25:26.84 +15:07:34.7: ref_mag=14.82 +/- 0.13 new_mean_mag=14.3297 delta=0.49 (need > 0.90)
Forced photometry on wcs_Leo-04-Q2b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:43:56.86 +17:56:26.3: 15.50 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.52 +/- 0.17
Forced photometry filter KEPT candidate at 09:43:56.86 +17:56:26.3: ref_mag=15.52 +/- 0.17 new_mean_mag=13.3765 delta=2.14 (need > 0.90)
Adding exclusion_list_local.txt__out31418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60080.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 8s
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Considering the candidate 59555_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59555_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59556_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59556_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59561_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59561_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59564_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59564_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59569_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59569_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59570_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59570_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59571_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59571_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59591_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59591_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
**** FOUND 09:21:00.92 +10:55:40.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59669_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59669_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59676_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59676_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
**** FOUND 09:40:58.95 +09:52:39.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 59739_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59739_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59765_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59765_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
**** FOUND 09:51:35.84 +17:28:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59770_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59770_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59842_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59842_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59848_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59848_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
**** FOUND 10:01:25.39 +15:40:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59900_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59900_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59903_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59903_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59931_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59931_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
**** FOUND 09:47:46.30 +10:05:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59935_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59935_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59949_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59949_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 59977_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 59977_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 59997_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 59997_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 60045_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 60045_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 60056_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 60056_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 60080_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
Preparing report for the candidate 60080_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
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Considering the candidate 60081_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 60081_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
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Considering the candidate 60082_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561
The candidate 60082_fd_Leo-04-Q2b1x1_2026-10-09_05-00-38_20.00sec_-0.00C_LIGHT_0561 did not pass the final checks
